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Timestamp:
04/03/08 12:44:50 (9 months ago)
Author:
gary
Message:

these changes affect the predicted iso sequence lines. there are three major parts:

cont_createmesh.cpp the fine continuum did not extend down to the wavelength of HeI 10830 so line overlap was not being treated. Extended low energy limit to below this line. this caused some asserted 10830 lines to change.

do not print H-like or He-like lines that are produced from collapsed levels. Their emission has problems which will be documented in a trac ticket.

the data/LineList* files had H and He like lines from collapsed levels commented out. The code now predicts far fewer lines from H and He like species.

iso_level - now keep track of whether the l-mixing collisions out of p are fast enough to mix the levels. if not a comment is printed saying that the H, He lines are not accurate

prt_alltau.cpp - do not print He I line optical depths twice

parse_atom_iso.cpp - add print levels option to atom H-like levels print or atom He-like levels print to print sizes of all ions of H and He sequence. the command does not change the number of levels.

Files:
1 modified

Legend:

Unmodified
Added
Removed
  • trunk/data/LineList_NLR.dat

    r13 r1913  
    133133Ca2k     3934 
    134134Ca2h     3969 
    135 h  1     3970     total H-epsilon 
     135#h  1     3970     total H-epsilon 
    136136S II     4070 
    137137S  2     4074 
     
    188188ca 2     8579 
    189189s  3     9069 
    190 H  1     9229 
     190#H  1     9229 
    191191s  3     9532 
    192 h  1     9546 
     192#h  1     9546 
    193193totl     9850 
    194194PA C     0 
     
    206206H  1     1.282m 
    207207H  1     1.094m 
    208 H  1     1.005m 
     208#H  1     1.005m 
    209209# 
    210210# Brackett series 
     
    212212H  1     4.051m 
    213213H  1     2.625m 
    214 H  1     2.166m  Brackett gamma 
    215 H  1     1.945m 
     214#H  1     2.166m  Brackett gamma 
     215#H  1     1.945m 
    216216# 
    217217# IR and coronal lines