Study of Magnetic Motions in the Solar Photosphere and Their Implications for Heating the Solar Atmosphere

Details Study of Magnetic Motions in the Solar Photosphere and Their Implications for Heating the Solar Atmosphere Study of Magnetic Motions in the Solar Photosphere and Their Implications for Heating the Solar Atmosphere

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996sao..rept.....n&link_type=abstract

Technical Report, Smithsonian Astrophysical Observatory Cambridge, MA United States

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Radiative Transfer, Solar Atmosphere, Photosphere, Chromosphere, Carbon Monoxide, Line Spectra, Solar Magnetic Field, Atmospheric Models, Atmospheric Heating, Frequency Distribution, Inhomogeneity, Lyman Alpha Radiation, Lyman Beta Radiation, Hydrogen, Solar Spectra, Molecular Spectra, Solar Temperature, Time Dependence, Dynamic Models, Stellar Activity, Applications Programs (Computers)

Scientific paper

Dynamic modeling of CO line formation, and the development of a
two-dimensional radiative transfer code that includes the effects of
partial frequency redistribution, are described.

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