Morphology and polarization of metric and decimetric solar radio pulsations: a statistical approach

Details Morphology and polarization of metric and decimetric solar radio pulsations: a statistical approach Morphology and polarization of metric and decimetric solar radio pulsations: a statistical approach

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..331m&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

6

Solar Flares, Solar Radio Bursts, Solar Radio Fine Structures, Radio Pulsations

Scientific paper

We analyzed a large data set of fine structures observed during type IV solar radio events recorded with high time resolution at single frequencies in the metric and decimetric bands by the Trieste Solar Radio System. Varieties of fine structures with periodical behavior but different temporal morphologies and polarization characteristics were identified. For selected events general statistics was derived in order to describe the evolution in time and at different observing frequencies, i.e. to infer the evolution of the related coronal plasma disturbances in time and height. To better characterize the observed radio pulsations in the framework of the flaring process, we derived the positions of the associated active regions, and studied the timing of such radio phenomena with respect to the associated SXR flares.

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