Abstract
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 non-flare-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 non-flare-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.
Published Version
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