Physical parameters in long-decay coronal enhancements

Details Physical parameters in long-decay coronal enhancements Physical parameters in long-decay coronal enhancements

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...61...69m&link_type=abstract

Solar Physics, vol. 61, Feb. 1979, p. 69-88.

Astronomy and Astrophysics

Astronomy

41

Plasma Decay, Solar Corona, Solar X-Rays, X Ray Imagery, Astronomical Maps, Skylab Program, X Ray Astronomy

Scientific paper

Four well-observed long-decay X-ray enhancements (LDEs) are examined which were associated with filament eruptions, white-light transients, and loop prominence systems. In each case the physical parameters of the X-ray-emitting plasma are determined, including the spatial distribution and temporal evolution of temperature and density. The results and recent analyses of other aspects of the four LDEs are compared with current models of loop prominence systems. It is concluded that only a magnetic-reconnection model, such as that proposed by Kopp and Pneuman (1976) is consistent with the observations.

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