Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...114..192m&link_type=abstract
Astronomy and Astrophysics, vol. 114, no. 1, Oct. 1982, p. 192-199. Research supported by the Institut National d'Astronomie et
Astronomy and Astrophysics
Astrophysics
8
Coronal Loops, Magnetic Flux, Magnetohydrodynamic Waves, Solar Magnetic Field, Solar Prominences, Doppler Effect, Magnetic Field Configurations, Radial Velocity, Solar Maximum Mission, Solar Spectra, Solar Spectrometers
Scientific paper
The active prominence of the 6 May 1980 has been observed between 5.23 and 10.22 UT with the Ultraviolet Spectrometer and Polarimeter (UVSP) on board the Solar Maximum Mission (SMM) satellite. Intensities of 1548 A line of CIV and dopplershifts have been derived. A motion of the magnetic tube maintaining the prominence material is noted. This motion is followed by a coronal transient observed with the Coronagraph and Polarimeter (C/P) between 11 and 13 UT. It is suggested that the event is related to a MHD wave induced by a flare occurring behind the solar disk, and a MHD modeling of the perturbation is proposed.
Mein Nicole
Schmieder Brigitte
Simon Gabor
Tandberg-Hanssen Einar
Wu Shi Tsan
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