The heating of filaments as a disappearance process

Details The heating of filaments as a disappearance process The heating of filaments as a disappearance process

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nascp2442..221m&link_type=abstract

In NASA. Goddard Space Flight Center Coronal and Prominence Plasmas p221-223 (SEE N87-20871 13-92)

Physics

6

Line Spectra, Solar Corona, Solar Heating, Solar Prominences, Solar Wind, Solar Physics, Spectrum Analysis, Stellar Mass Ejection, Ultraviolet Spectra

Scientific paper

The sudden disappearance of filaments, commonly called Disparition Brusque (DB) is of two types: (1) the well known ejection of cool prominence material in the corona, i.e., a dynamic process (BDd) and (2) the heating of the prominence plasma. When the hydrogen of the filament becomes ionised, then the filament start to be visible in EUV lines keeping the same shape and position as the cool one. This process which is a thermic disapperence was named DB thermic (DBt). Successive disappearances and condensations of a quiescent filament from 13 to 17 of June 1973 was studied. This observation was provided by two instruments on Skylab ATM satellite. These observations of disappearances and condensations are discussed.

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