Bursts with temporal fine structure at 5730 MHz

Details Bursts with temporal fine structure at 5730 MHz Bursts with temporal fine structure at 5730 MHz

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003soph..216..225l&link_type=abstract

Solar Physics, v. 216, Issue 1, p. 225-238 (2003).

Physics

3

Scientific paper

An analysis of solar radio bursts with temporal fine structure (TFS) at 5730 MHz in relation to the magnetic configuration of the corresponding active regions (AR) is presented. We found that the occurrence of TFS bursts increases with increasing complexity of the AR's magnetic configuration. The degree of polarization of TFS bursts varies over a wide range. Most of these fast bursts with a high degree of polarization were observed in active regions with a simple magnetic configuration β. Most of the unpolarized fast bursts were observed in active regions with the most complicated configuration βγδ. Because bursts that are polarized in different modes have different displacements of position with respect to that of associated microwave bursts, we conclude that there are at least two types of TFS bursts at 5730 MHz. We think that fast bursts that are polarized in the ordinary mode are due to microwave type III bursts.

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