Sudden disappearance of quiescent prominences

Details Sudden disappearance of quiescent prominences Sudden disappearance of quiescent prominences

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985rpspr...6...34a&link_type=abstract

In its USSR Rept.: Space (JPRS-USP-85-005) p 34 (SEE N86-14111 04-88) Transl. into ENGLISH from Astron. Zh. (Moscow), v. 61,

Astronomy and Astrophysics

Astronomy

H Alpha Line, Solar Prominences, Solar Radio Emission, Electron Density (Concentration), Plasma Density, Plasma Heating, Solar Magnetic Field, Solar Temperature

Scientific paper

Cases of the breakup of quiescent prominences on July 2, 1976, and July 30, 1980, are discussed. Radio and optical data at wavelengths 1.35 and 0.8 cm and in the H-alpha line, respectively, confirmed the arch structure of the prominences. The breakup took place both through expansion of the arch and as a consequence of plasma outflow through its bases, in which heat conduction played an insignificant role.

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