Statistics of Flaring Loops Observed by Nobeyama Radioheliograph. II. Spectral Evolution

Details Statistics of Flaring Loops Observed by Nobeyama Radioheliograph. II. Spectral Evolution Statistics of Flaring Loops Observed by Nobeyama Radioheliograph. II. Spectral Evolution

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009apj...702...19h&link_type=abstract

The Astrophysical Journal, Volume 702, Issue 1, pp. 19-26 (2009).

Astronomy and Astrophysics

Astronomy

6

Sun: Flares, Sun: Radio Radiation

Scientific paper

The spectral evolution of solar microwave bursts is studied in 10 impulsive events with loop-like structures, which are selected in the flare list of Nobeyama Radioheliograph. Most events have a brighter and harder looptop (LT) with maximum time later than at least one of its two footpoints (FPs), and have a common feature of the spectral evolution in the LT and the two FPs. There are five simple impulsive bursts with a well known pattern of soft-hard-soft or soft-hard-harder (SHH). It is first found that the other five events have multiple subpeaks in their impulsive phase, and mostly have a new feature of hard-soft-hard (HSH) in each subpeak, but, the well known tendency of SHH is still maintained in the total spectral evolution of these events. All of these features in the spectral evolution of the 10 selected events are consistent with the full Sun observations of Nobeyama Radio Polarimeters in these events. The new feature of HSH may be explained by the thermal free-free emission before, during, and after these bursts, together with multiple injections of nonthermal electrons, while the SHH pattern in the total duration may be directly caused by the trapping effect.

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