A simplified method for computing radiative energy loss due to spectral lines. 2: Programs for solar flare models

Details A simplified method for computing radiative energy loss due to spectral lines. 2: Programs for solar flare models A simplified method for computing radiative energy loss due to spectral lines. 2: Programs for solar flare models

Mar 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974erp..reptq....c&link_type=abstract

Environmental Research Papers Air Force Cambridge Research Labs., Hanscom AFB, MA.

Computer Science

Computer Programming, Energy Dissipation, Line Spectra, Models, Radiative Transfer, Solar Flares, Balmer Series, Computer Programs, Fortran, Lyman Spectra, Prediction Analysis Techniques, Solar Radiation

Scientific paper

The paper lists FORTRAN-IV programs that implement a simplified method
for computing radiative loss rates due to spectral lines. As it is
planned to apply these techniques to solar flare models, the programs
are set up to take into account Lyman alpha, Balmer-alpha and H-, the
principal contributors to radiative energy loss in solar flares.

Affiliated with

Also associated with

No associations

Rating

A simplified method for computing radiative energy loss due to spectral lines. 2: Programs for solar flare models does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A simplified method for computing radiative energy loss due to spectral lines. 2: Programs for solar flare models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A simplified method for computing radiative energy loss due to spectral lines. 2: Programs for solar flare models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1797042