Comments regarding energy release and transfer in solar flares

Details Comments regarding energy release and transfer in solar flares Comments regarding energy release and transfer in solar flares

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...53..271v&link_type=abstract

(International Astronomical Union, Meeting on How Can Flares Be Understood, Grenoble, France, Aug. 27, 1976.) Solar Physics, vol

Physics

Energy Transfer, Skylab Program, Solar Corona, Solar Flares, Solar X-Rays, Astronomical Models, High Temperature Plasmas, Solar Magnetic Field

Scientific paper

Skylab observations of the high-temperature coronal plasma are used in characterizing energy released in the corona during flare-like events. The loop structure of the soft X-ray flare features is reviewed; short-term exposures of several soft X-ray images are employed in suggesting that energy, and possibly material as well, is added to the apex of loop systems during flare events. An accompanying restriction in the flow of mass and energy from the loop apex is also hypothesized to account for the recorded observations. Further investigations of the confining ability of the magnetic fields that contain the X-ray emitting plasma are proposed.

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