Sudden disappearance and reappearance of solar filaments by heating and cooling

Details Sudden disappearance and reappearance of solar filaments by heating and cooling Sudden disappearance and reappearance of solar filaments by heating and cooling

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...230..474s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 230, no. 2, April 1990, p. 474-478.

Astronomy and Astrophysics

Astrophysics

3

Magnetic Field Configurations, Plasma Heating, Solar Corona, Solar Prominences, Solar Rotation, H Alpha Line, Solar Flares, Solar Magnetic Field, Spectroheliographs

Scientific paper

The sudden disappearance of filaments due to their heating is studied.
The observations were performed at Meudon with a three-wavelength
heliograph. It is shown that the thermal disappearance involves an
increase in plasma density.

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