Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005chjaa...5..508w&link_type=abstract
Chinese Journal of Astronomy and Astrophysics, Volume 5, Issue 5, pp. 508-518 (2005).
Astronomy and Astrophysics
Astrophysics
Scientific paper
We present a large complex radio burst and its associated fast time structures observed on 2001 April 10 in the frequency range of 0.65 7.6 GHz. The NoRH radio image observation shows very complex radio source structures which include preexisting, newly emerging, submerging/cancelling polarities and a bipolar, a tripolar (a `bipolar + remote unipolar'), and a quadrupolar structure. This suggests that the radio burst is generated from a very complicated loop structure. According to the spectral and image observations, we assume that the beginning of this flare was caused by a single bipolar loop configuration with a `Y-type' reconnection structure. A composite of radio continuum and fast time structures is contained in this flare. The various fast radio emission phenomena include normal and reverse drifting type III bursts, and slowly drifting and no-drift structures. The tripolar configurations may form a double-loop with a `three-legged' structure, which is an important source of the various types of fast time structures. The two-loop reconnection model can lead simultaneously to electron acceleration and corona heating. We have also analyzed the behaviors of coronal magnetic polarities and the emission processes of different types radio emission qualitatively. Interactions of a bipolar or multi-polar loop are consistent with our observational results. Our observations favor the magnetic reconnection configurations of the `inverted Y-type' (bipolar) and the `three-legged' structures (tripolar or quadrupolar).
Shi Shuo-Biao
Wang Min
Xie Rui-Xiang
Xu Chun
Yan Yi-Hua
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