Analysis of simultaneous SKYLAB and ground based flare observations

Details Analysis of simultaneous SKYLAB and ground based flare observations Analysis of simultaneous SKYLAB and ground based flare observations

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976stin...7726053k&link_type=abstract

Final Summary Report Lockheed Missiles and Space Co., Palo Alto, CA. Research Lab.

Computer Science

Data Reduction, Skylab Program, Solar Flares, Solar Observatories, Spectroheliographs, Absorption Spectra, Computer Programs, Line Spectra, Solar Electrons, Ultraviolet Spectrometers

Scientific paper

HeI and HeII resonance line data from Skylab were reduced, analyzed and compared with HeI D3 line intensities taken simultaneously from the Lockheed Rye Canyon Solar Observatory. Computer codes were developed for the calculation of total He line intensities and line profiles from model flare regions. These codes incorporate simultaneous solution of the line and continuum transport equations as needed together with the statistical equilibrium equations for a 30 level HeI, HeII, HeIII system. The energy level model consists of all terms through principal quantum number four. Interpretation of the observed data in terms of these parametric solutions and with simultaneous solution of the transport equations are discussed.

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