The derivation of the parameters of coronal mass motions from noise storm observations

Details The derivation of the parameters of coronal mass motions from noise storm observations The derivation of the parameters of coronal mass motions from noise storm observations

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..143..151b&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 143, no. 1, p. 151-172.

Physics

4

Coronal Loops, Noise Storms, Solar Corona, Solar Flares, Solar Spectra, Drift Rate, Solar Flux Density, Solar Limb

Scientific paper

Based on a total of 152 events, we studied the spectral parameters of the continuum component of isolated noise storms (Lantos, 1982) subdividing the data set according to flare-related and nonflare-related events. There were typical differences between both classes with regard to starting frequency and frequency extent. The flare-related events can mostly be attributed to loops rising into the corona with velocities as being known for transients of moderate velocity and erupting prominences. The nonflare-related events must evidently be ascribed to a broad variety of mass motions but on the average these mass motions have a lower outward drift velocity than those associated with the flare-related events.

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