fcwave = fudge factor to multiply the flux values below 257 angstrom: 1.
 iflux = which photon flux to use:  4 
 iseff = which set of cross sections to use:  8 
 WITHIN "FELINPROXY" WE FIRST READ IN THE CROSS SECTIONS FILE CRS_MARS.

 WITHIN "FELINPROXY" WE NOW CALCULATE THE SOLAR PHOTON FLUX ENERGY GRID

 WITHIN "FELINPROXY" WE NOW CALCULATE THE NORMALISED BRANCHING RATIOS

 WITHIN "FELINPROXY" WE NOW INTERPOLATE THE PHOTO CROSS SECTIONS ONTO THE SOLAR FLUX ENERGY GRID
 ATTENTION FUNCTION SEFINTPRO: THERE IS A POSSIBLE BUG BECAUSE ONE OF THE CROSS SECTIONS IS NEGATIVE:
 ---> VALUE             : -5.79E-05 (*1.0E-18[cm2])
 ---> TYPE              : 2 (1=Total, 2=Ionisation)
 ---> SPECIE            : 12 
 ---> SOLAR FLUX ENERGY :  5.43E+02[eV]
 ATTENTION FUNCTION SEFINTPRO: THERE IS A POSSIBLE BUG BECAUSE ONE OF THE CROSS SECTIONS IS NEGATIVE:
 ---> VALUE             : -2.21E-04 (*1.0E-18[cm2])
 ---> TYPE              : 2 (1=Total, 2=Ionisation)
 ---> SPECIE            : 13 
 ---> SOLAR FLUX ENERGY :  5.43E+02[eV]
 ATTENTION FUNCTION SEFINTPRO: THERE IS A POSSIBLE BUG BECAUSE ONE OF THE CROSS SECTIONS IS NEGATIVE:
 ---> VALUE             : -2.10E-04 (*1.0E-18[cm2])
 ---> TYPE              : 2 (1=Total, 2=Ionisation)
 ---> SPECIE            : 15 
 ---> SOLAR FLUX ENERGY :  5.43E+02[eV]

 FELINPROXY HAS ESSENTIALLY FINISHED, HERE IS IT'S OUTPUT
 ----------------------------------------------------
  
 AN "IPRT(5)" OUTPUT
 Normalized branching ratios for some of the photoion excited states the photoions can be excited to, interpolated onto the solar flux energy grid.
 Have all been printed to file: /tmp/tmp1JtVJx/Output_MarTIM_KINETIC_FELPROX_IPRT5