The corona associated with solar filaments

Details The corona associated with solar filaments The corona associated with solar filaments

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981soph...71..151c&link_type=abstract

Solar Physics, vol. 71, May 1981, p. 151-159.

Astronomy and Astrophysics

Astronomy

6

Line Spectra, Solar Corona, Solar Prominences, Solar Spectra, Ferric Ions, Filaments, H Alpha Line, Ion Emission, Photosphere, Solar Atmosphere, Solar Magnetic Field, Spectroheliographs, Sun, Ultraviolet Astronomy

Scientific paper

Spectroheliograms in high temperature ions such as Fe XV show the
existence of both filaments that are brighter than the ambient corona
and filaments that are darker than the ambient corona. The relationship
of the filaments to photospheric magnetograms is described, and a
possible physical mechanism to explain the differences is discussed.

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