Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977sva....21..476l&link_type=abstract
(Astronomicheskii Zhurnal, vol. 54, July-Aug. 1977, p. 841-845.) Soviet Astronomy, vol. 21, July-Aug. 1977, p. 476-478. Transla
Astronomy and Astrophysics
Astronomy
Plasma Radiation, Solar Corona, Solar Temperature, Solar X-Rays, X Ray Astronomy, Electron Density (Concentration), Scale Height, Stellar Models, Temperature Distribution, Vertical Distribution
Scientific paper
The temperature distribution in a nonflare solar X-ray source is derived from the observationally deduced exponential temperature dependence of plasma differential emission measure on the assumption of a barometric decrease in electron density with a constant scale height. An analytical model of the coronal X-ray source is developed on the basis of X-ray observations of a coronal condensation. The physical processes that cause a substantial density increase in the highest-temperature coronal filaments are briefly discussed.
Bulatov N. N.
Livshits Moisey A.
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