Studies on metric-decimetric Type II bursts in relation to soft X-ray flares

Details Studies on metric-decimetric Type II bursts in relation to soft X-ray flares Studies on metric-decimetric Type II bursts in relation to soft X-ray flares

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002soph..207..381d&link_type=abstract

Solar Physics, v. 207, Issue 2, p. 381-388 (2002).

Physics

1

Scientific paper

The relationship between metric type II radio bursts and soft X-ray (SXR) flares is studied. Type II bursts are highly associated with SXR flares. The duration and drift rate of type II bursts are found to depend on the duration, asymmetry in duration (ratio of rise time to duration), as well as on the peak flux of SXR bursts. Important results obtained are: (i) the durations of type II bursts are linearly correlated with the durations of associated SXR bursts in case of long-lived events (duration >40 min), whereas in short-lived flares such a correlation is not found, (ii) the durations of type II bursts do not depend upon the SXR peak flux, (iii) more durable type II radio bursts are correlated with more symmetric SXR bursts, (iv) average drift rates of type II bursts are larger in the events associated with more powerful and more symmetric SXR bursts.

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