This enables
the printing of many quantities which are defined locally at the last
spatial zone of the calculation. These include ion fractions, heating and cooling
rates, line and continuum emissivities and opacitites, execution times,
and level populations. They are printed to the log file, xout_step.log.
Default value is 0, and results in just the 500 brightest line luminosities (sorted by luminosity) and depths,
and the 500 brightest recombination continuum (sorted by luminosity)
luminosities and depths to be printed to the log file at the end of the run. With a value 1 many
additional quantities are printed, including ascii tables of total line and rrc luminosities and depths.
With a value of 2 in addition many useful local quantities such as ion fractions, thermal
rates, level populations are printed. Note that these local quantities are printed only at the final step of
the model run. With a value of 3 continuum luminosities and emissivities are printed.
With a value of 4 the list of lines is printed, along with upper and lower levels, transition probabilities
and statistical weights. With a value of 5 all rates affecting level populations, ionization, heating and
cooling internal to the code are also printed. These require significant familiarity with the
code. This switch affects only the ascii log file, xout_step.log. The standard fits output files
are unaffected by the value of lprint.
