The modeling of the solar upper photosphere and lower chromosphere based upon ATM data

Details The modeling of the solar upper photosphere and lower chromosphere based upon ATM data The modeling of the solar upper photosphere and lower chromosphere based upon ATM data

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982stin...8312033h&link_type=abstract

Unknown

Computer Science

Apollo Telescope Mount, Atmospheric Models, Chromosphere, Photosphere, Skylab Program, Autoionization, Digital Data, H Lines, Lyman Spectra, Photographs

Scientific paper

The use of the solar H I Lyman spectral line as a diagnostic of the
lower to middle chromosphere is discussed. Quiet sun Lyman profiles from
the photographic spectra were subjected to data reduction and
appropriate theoretical modelling was accomplished. Apollo telescope
mount data was utilized.

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