A solar prominence in H-alpha and X-rays

Details A solar prominence in H-alpha and X-rays A solar prominence in H-alpha and X-rays

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...234l...9p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 234, no. 1-2, Aug. 1990, p. L9-L11.

Astronomy and Astrophysics

Astrophysics

H Alpha Line, Solar Prominences, Solar X-Rays, Magnetohydrodynamics, Plasma Temperature, Solar Activity

Scientific paper

Rare multiwavelength observations of a solar prominence in May 1986 are presented. H-alpha and X-ray data are used to reveal properties of the cool and hot plasmas related to the prominence structure and activity. No X-ray emission is formed along the prominence cavity itself, which suggests a magnetically inert structure. X-rays are, however, associated with the footprint of the prominence, revealing the presence of hot plasma in loops adjacent to the prominence structure. These characteristics are examined in the light of previous solar prominence observations and models.

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