OUTPUT FILE FOR FELIN.F Latitude -90.0, 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 : 1.9856E+10 [eV/cm2/s] or : 3.1813E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -85.0, 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 : 4.0232E+10 [eV/cm2/s] or : 6.4459E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -80.0, 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 : 6.4560E+10 [eV/cm2/s] or : 1.0344E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -75.0, 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 : 9.0256E+10 [eV/cm2/s] or : 1.4461E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -70.0, 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 : 1.1624E+11 [eV/cm2/s] or : 1.8624E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -65.0, 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 : 1.4190E+11 [eV/cm2/s] or : 2.2735E-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 : 1.6680E+11 [eV/cm2/s] or : 2.6724E-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 : 1.9066E+11 [eV/cm2/s] or : 3.0548E-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 : 2.1322E+11 [eV/cm2/s] or : 3.4163E-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 : 2.3427E+11 [eV/cm2/s] or : 3.7535E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -40.0, 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 : 2.5324E+11 [eV/cm2/s] or : 4.0574E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -35.0, 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 : 2.7058E+11 [eV/cm2/s] or : 4.3353E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -30.0, 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 : 2.8596E+11 [eV/cm2/s] or : 4.5816E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -25.0, 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 : 2.9918E+11 [eV/cm2/s] or : 4.7934E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -20.0, 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 : 3.1012E+11 [eV/cm2/s] or : 4.9688E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -15.0, 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 : 3.1873E+11 [eV/cm2/s] or : 5.1067E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -10.0, 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 : 3.2493E+11 [eV/cm2/s] or : 5.2060E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -5.0, 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 : 3.2866E+11 [eV/cm2/s] or : 5.2658E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 0.0, 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 : 3.2990E+11 [eV/cm2/s] or : 5.2857E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 5.0, 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 : 3.2864E+11 [eV/cm2/s] or : 5.2655E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 10.0, 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 : 3.2490E+11 [eV/cm2/s] or : 5.2055E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 15.0, 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 : 3.1869E+11 [eV/cm2/s] or : 5.1061E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 20.0, 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 : 3.1007E+11 [eV/cm2/s] or : 4.9680E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 25.0, 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 : 2.9912E+11 [eV/cm2/s] or : 4.7925E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 30.0, 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 : 2.8591E+11 [eV/cm2/s] or : 4.5808E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 35.0, 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 : 2.7055E+11 [eV/cm2/s] or : 4.3348E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 40.0, 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 : 2.5322E+11 [eV/cm2/s] or : 4.0571E-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 : 2.3419E+11 [eV/cm2/s] or : 3.7522E-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 : 2.1328E+11 [eV/cm2/s] or : 3.4172E-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 : 1.9075E+11 [eV/cm2/s] or : 3.0563E-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 : 1.6692E+11 [eV/cm2/s] or : 2.6744E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 65.0, 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 : 1.4204E+11 [eV/cm2/s] or : 2.2757E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 70.0, 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 : 1.1640E+11 [eV/cm2/s] or : 1.8650E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 75.0, 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 : 9.0440E+10 [eV/cm2/s] or : 1.4490E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 80.0, 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 : 6.4762E+10 [eV/cm2/s] or : 1.0376E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 85.0, 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 : 4.0448E+10 [eV/cm2/s] or : 6.4806E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 90.0, 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 : 2.0061E+10 [eV/cm2/s] or : 3.2142E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -90.0, 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 : 1.9856E+10 [eV/cm2/s] or : 3.1813E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -85.0, 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 : 3.8141E+10 [eV/cm2/s] or : 6.1110E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -80.0, 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 : 5.9924E+10 [eV/cm2/s] or : 9.6010E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -75.0, 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 : 8.3008E+10 [eV/cm2/s] or : 1.3299E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -70.0, 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 : 1.0642E+11 [eV/cm2/s] or : 1.7050E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -65.0, 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 : 1.2958E+11 [eV/cm2/s] or : 2.0761E-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 : 1.5211E+11 [eV/cm2/s] or : 2.4370E-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 : 1.7370E+11 [eV/cm2/s] or : 2.7830E-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 : 1.9413E+11 [eV/cm2/s] or : 3.1104E-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 : 2.1320E+11 [eV/cm2/s] or : 3.4158E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -40.0, 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 : 2.3072E+11 [eV/cm2/s] or : 3.6967E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -35.0, 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 : 2.4626E+11 [eV/cm2/s] or : 3.9456E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -30.0, 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 : 2.6008E+11 [eV/cm2/s] or : 4.1670E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -25.0, 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 : 2.7205E+11 [eV/cm2/s] or : 4.3588E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -20.0, 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 : 2.8199E+11 [eV/cm2/s] or : 4.5180E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -15.0, 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 : 2.8980E+11 [eV/cm2/s] or : 4.6432E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -10.0, 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 : 2.9542E+11 [eV/cm2/s] or : 4.7332E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -5.0, 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 : 2.9880E+11 [eV/cm2/s] or : 4.7874E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 0.0, 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 : 2.9992E+11 [eV/cm2/s] or : 4.8054E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 5.0, 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 : 2.9878E+11 [eV/cm2/s] or : 4.7870E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 10.0, 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 : 2.9537E+11 [eV/cm2/s] or : 4.7324E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 15.0, 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 : 2.8974E+11 [eV/cm2/s] or : 4.6422E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 20.0, 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 : 2.8191E+11 [eV/cm2/s] or : 4.5168E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 25.0, 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 : 2.7195E+11 [eV/cm2/s] or : 4.3573E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 30.0, 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 : 2.5998E+11 [eV/cm2/s] or : 4.1654E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 35.0, 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 : 2.4616E+11 [eV/cm2/s] or : 3.9440E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 40.0, 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 : 2.3065E+11 [eV/cm2/s] or : 3.6955E-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 : 2.1316E+11 [eV/cm2/s] or : 3.4152E-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 : 1.9413E+11 [eV/cm2/s] or : 3.1104E-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 : 1.7374E+11 [eV/cm2/s] or : 2.7837E-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 : 1.5218E+11 [eV/cm2/s] or : 2.4383E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 65.0, 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 : 1.2969E+11 [eV/cm2/s] or : 2.0780E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 70.0, 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 : 1.0656E+11 [eV/cm2/s] or : 1.7074E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 75.0, 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 : 8.3180E+10 [eV/cm2/s] or : 1.3327E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 80.0, 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 : 6.0119E+10 [eV/cm2/s] or : 9.6323E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 85.0, 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 : 3.8355E+10 [eV/cm2/s] or : 6.1452E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 90.0, 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 : 2.0061E+10 [eV/cm2/s] or : 3.2142E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -90.0, 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 : 1.9856E+10 [eV/cm2/s] or : 3.1813E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -85.0, 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 : 3.5931E+10 [eV/cm2/s] or : 5.7569E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -80.0, 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 : 5.5009E+10 [eV/cm2/s] or : 8.8135E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -75.0, 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 : 7.5296E+10 [eV/cm2/s] or : 1.2064E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -70.0, 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 : 9.5948E+10 [eV/cm2/s] or : 1.5373E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -65.0, 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 : 1.1643E+11 [eV/cm2/s] or : 1.8654E-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 : 1.3638E+11 [eV/cm2/s] or : 2.1851E-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 : 1.5553E+11 [eV/cm2/s] or : 2.4919E-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 : 1.7366E+11 [eV/cm2/s] or : 2.7824E-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 : 1.9058E+11 [eV/cm2/s] or : 3.0535E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -40.0, 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 : 2.0615E+11 [eV/cm2/s] or : 3.3029E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -35.0, 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 : 2.2021E+11 [eV/cm2/s] or : 3.5281E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -30.0, 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 : 2.3263E+11 [eV/cm2/s] or : 3.7272E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -25.0, 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 : 2.4304E+11 [eV/cm2/s] or : 3.8939E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -20.0, 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 : 2.5181E+11 [eV/cm2/s] or : 4.0345E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -15.0, 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 : 2.5872E+11 [eV/cm2/s] or : 4.1452E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -10.0, 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 : 2.6370E+11 [eV/cm2/s] or : 4.2251E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -5.0, 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 : 2.6672E+11 [eV/cm2/s] or : 4.2734E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 0.0, 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 : 2.6772E+11 [eV/cm2/s] or : 4.2895E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 5.0, 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 : 2.6670E+11 [eV/cm2/s] or : 4.2730E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 10.0, 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 : 2.6366E+11 [eV/cm2/s] or : 4.2243E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 15.0, 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 : 2.5864E+11 [eV/cm2/s] or : 4.1440E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 20.0, 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 : 2.5171E+11 [eV/cm2/s] or : 4.0329E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 25.0, 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 : 2.4292E+11 [eV/cm2/s] or : 3.8921E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 30.0, 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 : 2.3235E+11 [eV/cm2/s] or : 3.7227E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 35.0, 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 : 2.2008E+11 [eV/cm2/s] or : 3.5262E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 40.0, 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 : 2.0604E+11 [eV/cm2/s] or : 3.3012E-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 : 1.9050E+11 [eV/cm2/s] or : 3.0523E-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 : 1.7362E+11 [eV/cm2/s] or : 2.7817E-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 : 1.5553E+11 [eV/cm2/s] or : 2.4919E-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 : 1.3642E+11 [eV/cm2/s] or : 2.1857E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 65.0, 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 : 1.1651E+11 [eV/cm2/s] or : 1.8667E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 70.0, 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 : 9.6073E+10 [eV/cm2/s] or : 1.5393E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 75.0, 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 : 7.5462E+10 [eV/cm2/s] or : 1.2091E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 80.0, 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 : 5.5201E+10 [eV/cm2/s] or : 8.8444E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 85.0, 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 : 3.6142E+10 [eV/cm2/s] or : 5.7907E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 90.0, 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 : 2.0061E+10 [eV/cm2/s] or : 3.2142E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -90.0, 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 : 1.9856E+10 [eV/cm2/s] or : 3.1813E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -85.0, 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 : 3.3630E+10 [eV/cm2/s] or : 5.3882E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -80.0, 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 : 4.9882E+10 [eV/cm2/s] or : 7.9921E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -75.0, 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 : 6.7223E+10 [eV/cm2/s] or : 1.0770E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -70.0, 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 : 8.4944E+10 [eV/cm2/s] or : 1.3610E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -65.0, 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 : 1.0258E+11 [eV/cm2/s] or : 1.6435E-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 : 1.1980E+11 [eV/cm2/s] or : 1.9194E-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 : 1.3634E+11 [eV/cm2/s] or : 2.1845E-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 : 1.5202E+11 [eV/cm2/s] or : 2.4356E-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 : 1.6666E+11 [eV/cm2/s] or : 2.6702E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -40.0, 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 : 1.8013E+11 [eV/cm2/s] or : 2.8861E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -35.0, 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 : 1.9231E+11 [eV/cm2/s] or : 3.0812E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -30.0, 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 : 2.0308E+11 [eV/cm2/s] or : 3.2537E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -25.0, 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 : 2.1235E+11 [eV/cm2/s] or : 3.4023E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -20.0, 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 : 2.2005E+11 [eV/cm2/s] or : 3.5256E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -15.0, 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 : 2.2610E+11 [eV/cm2/s] or : 3.6225E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -10.0, 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 : 2.3046E+11 [eV/cm2/s] or : 3.6924E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude -5.0, 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 : 2.3292E+11 [eV/cm2/s] or : 3.7319E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 0.0, 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 : 2.3379E+11 [eV/cm2/s] or : 3.7458E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 5.0, 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 : 2.3289E+11 [eV/cm2/s] or : 3.7314E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 10.0, 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 : 2.3035E+11 [eV/cm2/s] or : 3.6907E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 15.0, 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 : 2.2603E+11 [eV/cm2/s] or : 3.6214E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 20.0, 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 : 2.1995E+11 [eV/cm2/s] or : 3.5240E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 25.0, 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 : 2.1223E+11 [eV/cm2/s] or : 3.4003E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 30.0, 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 : 2.0294E+11 [eV/cm2/s] or : 3.2516E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 35.0, 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 : 1.9217E+11 [eV/cm2/s] or : 3.0790E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 40.0, 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 : 1.8000E+11 [eV/cm2/s] or : 2.8840E-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 : 1.6655E+11 [eV/cm2/s] or : 2.6684E-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 : 1.5193E+11 [eV/cm2/s] or : 2.4343E-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 : 1.3630E+11 [eV/cm2/s] or : 2.1837E-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 : 1.1979E+11 [eV/cm2/s] or : 1.9193E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 65.0, 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 : 1.0263E+11 [eV/cm2/s] or : 1.6444E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 70.0, 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 : 8.5053E+10 [eV/cm2/s] or : 1.3627E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 75.0, 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 : 6.7380E+10 [eV/cm2/s] or : 1.0796E-01 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 80.0, 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 : 5.0073E+10 [eV/cm2/s] or : 8.0227E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 85.0, 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 : 3.3840E+10 [eV/cm2/s] or : 5.4219E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED OUTPUT FILE FOR FELIN.F Latitude 90.0, 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 : 2.0061E+10 [eV/cm2/s] or : 3.2142E-02 [erg/cm2/s] FELIN.F COMPLETELY FINISHED