A model for X-ray emission from loop prominences

Details A model for X-ray emission from loop prominences A model for X-ray emission from loop prominences

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...53...41p&link_type=abstract

Solar Physics, vol. 53, July 1977, p. 41-58.

Physics

1

Astronomical Models, Line Spectra, Solar Prominences, Solar X-Rays, Chromosphere, H Alpha Line, Magnetic Flux, Plasma Heating, Solar Flares

Scientific paper

A study is made of X-ray line emission observed during the developing stages of a set of post-flare loop prominences. The time behavior of the line emission can be described by a model consisting of two flux tubes containing plasma heated impulsively at the flash phase; the plasma cools by radiation and by conduction to the chromosphere. These ideas are extended to the possible formation of H-alpha prominences from low-lying hot loops.

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