Physics
Scientific paper
Oct 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...80..279m&link_type=abstract
Solar Physics, vol. 80, Oct. 1982, p. 279-294.
Physics
6
Line Spectra, Solar Prominences, Solar Velocity, D Lines, H Alpha Line, Kinetic Energy, Line Of Sight, Radiant Flux Density, Solar Magnetic Field
Scientific paper
Observations of quiescent prominences with the Zeiss Universal Birefringent Filter at Sacramento Peak show short-lived brightenings and velocity transients in H-alpha and D3. The larger events range in area from 25 to 170 square arc sec, have lifetimes of approximately 30 min, velocities of 30 km/s, and total energy excesses up to 7 x 10 to the 27th ergs. These events do not disrupt the stable structure of the prominence, and are interpreted as either condensation events or low energy flares.
Malville Mckim J.
Toot David G.
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