Output files of the emergent flux

These files contain the emergent flux at the uppermost depth point (emflux.lst), the flux at the Rosseland optical depth of 2/3 (formflux.lst), and at the innermost depth point (ndflux.lst). In addition, the file emflux.lst contains the values of equivalent width for each line. The output is controlled by variables LPEMFL (emflux.lst), LPFOFL (formflux.lst), LPNDFL (ndflux.lst).

IJ, FREQ(IJ), ALAM, AH(IJ,1), LOG10(AH(IJ,1))

FORMAT (I5,1P3D15.7,0PF9.3)

ITR, ILOW(ITR), IUP(ITR), IPROF(ITR), EW, NFLINE(ITR)

FORMAT (3I5,I6,0PF13.6,I7)

1 line for each frequency point for all three files:

index of the frequency point

FREQ(IJ)

frequency (in s^-1)

ALAM

wavelength in Angstroms

AJ(IJ,1)*FHU(IJ) or AH(IJ,NDRE) or AH(IJ,ND)

emergent flux at the uppermost depth point, flux at tau_R=2/3, flux at the innermost depth point, respectively

LOG10(AJ(IJ,1)*FHU(IJ))

or LOG10(AH(IJ,NDRE)) or LOG10(AH(IJ,ND))

logarithm of flux from the preceding value

1 line for each line transition (only for emflux.lst):

ITR

index of the transition

ILOW(ITR)

index of the lower level

IUP(ITR)

index of the upper level

IPROF(ITR)

index of the line profile

equivalent width in Angstroms

NFLINE(ITR)

number of frequency points in a line

Back to the main page of the code ATA
Last update: 27.8.2001