OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 0.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.3412E+11 [eV/cm2/s]
or : 5.3533E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 0.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.0429E+11 [eV/cm2/s]
or : 4.8753E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 0.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.7221E+11 [eV/cm2/s]
or : 4.3614E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 0.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.3822E+11 [eV/cm2/s]
or : 3.8167E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 5.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.3284E+11 [eV/cm2/s]
or : 5.3328E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 5.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.0313E+11 [eV/cm2/s]
or : 4.8567E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 5.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.7118E+11 [eV/cm2/s]
or : 4.3449E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 5.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.3733E+11 [eV/cm2/s]
or : 3.8025E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 10.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.2909E+11 [eV/cm2/s]
or : 5.2727E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 10.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.9970E+11 [eV/cm2/s]
or : 4.8017E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 10.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.6814E+11 [eV/cm2/s]
or : 4.2961E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 10.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.3469E+11 [eV/cm2/s]
or : 3.7603E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 15.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.2287E+11 [eV/cm2/s]
or : 5.1731E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 15.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.9405E+11 [eV/cm2/s]
or : 4.7113E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 15.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.6311E+11 [eV/cm2/s]
or : 4.2155E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 15.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.3034E+11 [eV/cm2/s]
or : 3.6905E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 20.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.1423E+11 [eV/cm2/s]
or : 5.0347E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 20.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.8623E+11 [eV/cm2/s]
or : 4.5860E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 20.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.5614E+11 [eV/cm2/s]
or : 4.1038E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 20.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.2431E+11 [eV/cm2/s]
or : 3.5939E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 25.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.0327E+11 [eV/cm2/s]
or : 4.8590E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 25.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.7628E+11 [eV/cm2/s]
or : 4.4265E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 25.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.4728E+11 [eV/cm2/s]
or : 3.9619E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 25.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.1665E+11 [eV/cm2/s]
or : 3.4712E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 30.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.9005E+11 [eV/cm2/s]
or : 4.6472E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 30.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.6427E+11 [eV/cm2/s]
or : 4.2342E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 30.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.3663E+11 [eV/cm2/s]
or : 3.7912E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 30.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.0744E+11 [eV/cm2/s]
or : 3.3236E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 35.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.7469E+11 [eV/cm2/s]
or : 4.4011E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 35.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.5034E+11 [eV/cm2/s]
or : 4.0109E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 35.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.2427E+11 [eV/cm2/s]
or : 3.5932E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 35.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.9676E+11 [eV/cm2/s]
or : 3.1525E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 40.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.5730E+11 [eV/cm2/s]
or : 4.1225E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 40.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.3460E+11 [eV/cm2/s]
or : 3.7588E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 40.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.1032E+11 [eV/cm2/s]
or : 3.3698E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 40.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.8472E+11 [eV/cm2/s]
or : 2.9596E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 45.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.3807E+11 [eV/cm2/s]
or : 3.8144E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 45.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.1722E+11 [eV/cm2/s]
or : 3.4803E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 45.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.9493E+11 [eV/cm2/s]
or : 3.1231E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 45.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.7144E+11 [eV/cm2/s]
or : 2.7468E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 50.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.1720E+11 [eV/cm2/s]
or : 3.4800E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 50.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.9836E+11 [eV/cm2/s]
or : 3.1781E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 50.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.7824E+11 [eV/cm2/s]
or : 2.8557E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 50.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.5706E+11 [eV/cm2/s]
or : 2.5164E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 55.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.9489E+11 [eV/cm2/s]
or : 3.1226E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 55.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.7822E+11 [eV/cm2/s]
or : 2.8555E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 55.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.6043E+11 [eV/cm2/s]
or : 2.5705E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 55.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.4174E+11 [eV/cm2/s]
or : 2.2709E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 60.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.7140E+11 [eV/cm2/s]
or : 2.7462E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 60.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.5704E+11 [eV/cm2/s]
or : 2.5161E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 60.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.4173E+11 [eV/cm2/s]
or : 2.2708E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 60.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.2567E+11 [eV/cm2/s]
or : 2.0134E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 65.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.4702E+11 [eV/cm2/s]
or : 2.3556E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 65.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.3508E+11 [eV/cm2/s]
or : 2.1643E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 65.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.2238E+11 [eV/cm2/s]
or : 1.9608E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 65.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.0907E+11 [eV/cm2/s]
or : 1.7476E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 70.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.2212E+11 [eV/cm2/s]
or : 1.9566E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 70.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.1270E+11 [eV/cm2/s]
or : 1.8057E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 70.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.0269E+11 [eV/cm2/s]
or : 1.6453E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 70.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 9.2225E+10 [eV/cm2/s]
or : 1.4776E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 75.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 9.7177E+10 [eV/cm2/s]
or : 1.5570E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 75.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 9.0318E+10 [eV/cm2/s]
or : 1.4471E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 75.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 8.3045E+10 [eV/cm2/s]
or : 1.3306E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 75.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 7.5454E+10 [eV/cm2/s]
or : 1.2089E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 80.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 7.2850E+10 [eV/cm2/s]
or : 1.1672E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 80.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 6.8536E+10 [eV/cm2/s]
or : 1.0981E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 80.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 6.3964E+10 [eV/cm2/s]
or : 1.0248E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 80.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 5.9192E+10 [eV/cm2/s]
or : 9.4838E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 85.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 5.0150E+10 [eV/cm2/s]
or : 8.0350E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 85.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 4.8226E+10 [eV/cm2/s]
or : 7.7268E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 85.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 4.6175E+10 [eV/cm2/s]
or : 7.3982E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 85.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 4.4021E+10 [eV/cm2/s]
or : 7.0530E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 90.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.0702E+10 [eV/cm2/s]
or : 4.9191E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 90.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.0716E+10 [eV/cm2/s]
or : 4.9213E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 90.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.0717E+10 [eV/cm2/s]
or : 4.9215E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 90.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.0703E+10 [eV/cm2/s]
or : 4.9192E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 95.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.6064E+10 [eV/cm2/s]
or : 2.5738E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 95.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.7192E+10 [eV/cm2/s]
or : 2.7545E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 95.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.8444E+10 [eV/cm2/s]
or : 2.9551E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 95.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.9819E+10 [eV/cm2/s]
or : 3.1754E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 100.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 6.7690E+09 [eV/cm2/s]
or : 1.0845E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 100.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 8.0968E+09 [eV/cm2/s]
or : 1.2973E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 100.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 9.7011E+09 [eV/cm2/s]
or : 1.5543E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 100.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.1611E+10 [eV/cm2/s]
or : 1.8603E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 105.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.0636E+09 [eV/cm2/s]
or : 3.3063E-03 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 105.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.0091E+09 [eV/cm2/s]
or : 4.8213E-03 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 105.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 4.3122E+09 [eV/cm2/s]
or : 6.9091E-03 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 105.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 6.0651E+09 [eV/cm2/s]
or : 9.7175E-03 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 110.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.9969E+08 [eV/cm2/s]
or : 4.8017E-04 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 110.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 7.2243E+08 [eV/cm2/s]
or : 1.1575E-03 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 110.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.4838E+09 [eV/cm2/s]
or : 2.3774E-03 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 110.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.7264E+09 [eV/cm2/s]
or : 4.3683E-03 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 115.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 6.6485E+06 [eV/cm2/s]
or : 1.0652E-05 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 115.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 5.5468E+07 [eV/cm2/s]
or : 8.8872E-05 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 115.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.9552E+08 [eV/cm2/s]
or : 4.7348E-04 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 115.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 9.6128E+08 [eV/cm2/s]
or : 1.5402E-03 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 120.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 4.9360E+05 [eV/cm2/s]
or : 7.9085E-07 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 120.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.8454E+07 [eV/cm2/s]
or : 2.9567E-05 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 120.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.0553E+08 [eV/cm2/s]
or : 3.2931E-04 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 125.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.2935E+05 [eV/cm2/s]
or : 2.0724E-07 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 125.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.8574E+07 [eV/cm2/s]
or : 2.9759E-05 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 130.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 5.0414E+05 [eV/cm2/s]
or : 8.0773E-07 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 230.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.7755E+05 [eV/cm2/s]
or : 6.0491E-07 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 235.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 8.0489E+04 [eV/cm2/s]
or : 1.2896E-07 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 235.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.6211E+07 [eV/cm2/s]
or : 2.5973E-05 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 240.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.1480E+05 [eV/cm2/s]
or : 5.0437E-07 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 240.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.5554E+07 [eV/cm2/s]
or : 2.4920E-05 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 240.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.9382E+08 [eV/cm2/s]
or : 3.1054E-04 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 245.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 4.8918E+06 [eV/cm2/s]
or : 7.8376E-06 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 245.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 4.8674E+07 [eV/cm2/s]
or : 7.7985E-05 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 245.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.7513E+08 [eV/cm2/s]
or : 4.4082E-04 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 245.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 8.9462E+08 [eV/cm2/s]
or : 1.4334E-03 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 250.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.7300E+08 [eV/cm2/s]
or : 4.3740E-04 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 250.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 6.6305E+08 [eV/cm2/s]
or : 1.0623E-03 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 250.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.3627E+09 [eV/cm2/s]
or : 2.1833E-03 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 250.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.5174E+09 [eV/cm2/s]
or : 4.0334E-03 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 255.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.8796E+09 [eV/cm2/s]
or : 3.0115E-03 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 255.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.7506E+09 [eV/cm2/s]
or : 4.4070E-03 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 255.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.9679E+09 [eV/cm2/s]
or : 6.3574E-03 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 255.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 5.6395E+09 [eV/cm2/s]
or : 9.0356E-03 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 260.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 6.2765E+09 [eV/cm2/s]
or : 1.0056E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 260.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 7.5353E+09 [eV/cm2/s]
or : 1.2073E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 260.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 9.0848E+09 [eV/cm2/s]
or : 1.4556E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 260.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.0968E+10 [eV/cm2/s]
or : 1.7574E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 265.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.5338E+10 [eV/cm2/s]
or : 2.4575E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 265.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.6422E+10 [eV/cm2/s]
or : 2.6311E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 265.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.7660E+10 [eV/cm2/s]
or : 2.8295E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 265.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.9057E+10 [eV/cm2/s]
or : 3.0532E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 270.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.0081E+10 [eV/cm2/s]
or : 4.8196E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 270.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.0042E+10 [eV/cm2/s]
or : 4.8133E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 270.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.0022E+10 [eV/cm2/s]
or : 4.8102E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 270.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.0027E+10 [eV/cm2/s]
or : 4.8110E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 275.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 4.9701E+10 [eV/cm2/s]
or : 7.9630E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 275.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 4.7691E+10 [eV/cm2/s]
or : 7.6411E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 275.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 4.5584E+10 [eV/cm2/s]
or : 7.3034E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 275.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 4.3410E+10 [eV/cm2/s]
or : 6.9551E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 280.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 7.2643E+10 [eV/cm2/s]
or : 1.1639E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 280.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 6.8226E+10 [eV/cm2/s]
or : 1.0931E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 280.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 6.3570E+10 [eV/cm2/s]
or : 1.0185E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 280.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 5.8742E+10 [eV/cm2/s]
or : 9.4117E-02 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 285.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 9.7164E+10 [eV/cm2/s]
or : 1.5568E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 285.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 9.0196E+10 [eV/cm2/s]
or : 1.4451E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 285.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 8.2825E+10 [eV/cm2/s]
or : 1.3270E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 285.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 7.5155E+10 [eV/cm2/s]
or : 1.2041E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 290.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.2225E+11 [eV/cm2/s]
or : 1.9587E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 290.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.1272E+11 [eV/cm2/s]
or : 1.8060E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 290.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.0261E+11 [eV/cm2/s]
or : 1.6440E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 290.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 9.2054E+10 [eV/cm2/s]
or : 1.4749E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 295.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.4725E+11 [eV/cm2/s]
or : 2.3593E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 295.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.3521E+11 [eV/cm2/s]
or : 2.1664E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 295.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.2241E+11 [eV/cm2/s]
or : 1.9612E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 295.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.0901E+11 [eV/cm2/s]
or : 1.7465E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 300.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.7170E+11 [eV/cm2/s]
or : 2.7510E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 300.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.5724E+11 [eV/cm2/s]
or : 2.5193E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 300.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.4184E+11 [eV/cm2/s]
or : 2.2725E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 300.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.2568E+11 [eV/cm2/s]
or : 2.0136E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 305.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.9523E+11 [eV/cm2/s]
or : 3.1280E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 305.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.7848E+11 [eV/cm2/s]
or : 2.8595E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 305.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.6060E+11 [eV/cm2/s]
or : 2.5731E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 305.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.4181E+11 [eV/cm2/s]
or : 2.2720E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 310.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.1756E+11 [eV/cm2/s]
or : 3.4857E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 310.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.9864E+11 [eV/cm2/s]
or : 3.1826E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 310.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.7843E+11 [eV/cm2/s]
or : 2.8589E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 310.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.5717E+11 [eV/cm2/s]
or : 2.5181E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 315.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.3844E+11 [eV/cm2/s]
or : 3.8202E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 315.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.1751E+11 [eV/cm2/s]
or : 3.4850E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 315.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.9514E+11 [eV/cm2/s]
or : 3.1266E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 315.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.7157E+11 [eV/cm2/s]
or : 2.7490E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 320.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.5765E+11 [eV/cm2/s]
or : 4.1281E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 320.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.3489E+11 [eV/cm2/s]
or : 3.7635E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 320.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.1055E+11 [eV/cm2/s]
or : 3.3734E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 320.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.8487E+11 [eV/cm2/s]
or : 2.9620E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 325.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.7502E+11 [eV/cm2/s]
or : 4.4064E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 325.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.5061E+11 [eV/cm2/s]
or : 4.0153E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 325.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.2448E+11 [eV/cm2/s]
or : 3.5967E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 325.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 1.9691E+11 [eV/cm2/s]
or : 3.1549E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 330.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.9035E+11 [eV/cm2/s]
or : 4.6520E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 330.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.6453E+11 [eV/cm2/s]
or : 4.2382E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 330.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.3683E+11 [eV/cm2/s]
or : 3.7945E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 330.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.0758E+11 [eV/cm2/s]
or : 3.3259E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 335.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.0353E+11 [eV/cm2/s]
or : 4.8632E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 335.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.7650E+11 [eV/cm2/s]
or : 4.4301E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 335.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.4746E+11 [eV/cm2/s]
or : 3.9648E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 335.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.1678E+11 [eV/cm2/s]
or : 3.4733E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 340.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.1445E+11 [eV/cm2/s]
or : 5.0381E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 340.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.8642E+11 [eV/cm2/s]
or : 4.5890E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 340.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.5629E+11 [eV/cm2/s]
or : 4.1062E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 340.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.2442E+11 [eV/cm2/s]
or : 3.5956E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 345.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.2304E+11 [eV/cm2/s]
or : 5.1757E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 345.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.9420E+11 [eV/cm2/s]
or : 4.7136E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 345.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.6323E+11 [eV/cm2/s]
or : 4.2174E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 345.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.3043E+11 [eV/cm2/s]
or : 3.6919E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 350.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.2921E+11 [eV/cm2/s]
or : 5.2745E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 350.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.9979E+11 [eV/cm2/s]
or : 4.8033E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 350.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.6822E+11 [eV/cm2/s]
or : 4.2974E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 350.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.3475E+11 [eV/cm2/s]
or : 3.7612E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 45.0, longitude 355.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.3290E+11 [eV/cm2/s]
or : 5.3337E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 50.0, longitude 355.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 3.0317E+11 [eV/cm2/s]
or : 4.8575E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 55.0, longitude 355.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.7122E+11 [eV/cm2/s]
or : 4.3455E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED
OUTPUT FILE FOR FELIN.F
Latitude 60.0, longitude 355.0.
WITHIN SUBROUTINE SETPAR WE FIRST SORT OUT THE USER INPUT DATA FROM "MASTER_IN".
iprt = what else is to be printed in this file: 0 0 0 0 0 0 0 0 0 0 0 0 0 0
imod = how to divide up the energy grid: 1
WITHIN SUBROUTINE SETPAR WE NOW CALCULATE THE CHAPMAN FUNCTION
WITHIN SUBROUTINE DEPO WE WILL COMPUTE THE PRIMARY PHOTOELECTRON PRODUCTION.
WITHIN SUBROUTINE FELIN.F WE NOW WRITE OUT EVERYTHING CALCULATED.
The total energy from photoelectron production is : 2.3736E+11 [eV/cm2/s]
or : 3.8030E-01 [erg/cm2/s]
FELIN.F COMPLETELY FINISHED