Solar Radio Bursts in the Period Oct. 22-Nov. 4, 2003

A series of solar radio bursts were observed in AR NOAA 10486 with the Solar Broadband (1.1-7.6 GHz) Radio Spectrometers (SBRS of China). Here we analyze four significant events associated with CME events and strong X-ray flares that occurred on 2003 October 22, 26, 27, 29. The Oct. 26 event is a lo...

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Veröffentlicht in:Chinese journal of astronomy and astrophysics 2004-06, Vol.4 (3), p.205-208
Hauptverfasser: Tan, Cheng-Ming, Fu, Qi-Jun, Yan, Yi-Hua, Liu, Yu-Ying
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Sprache:eng
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Zusammenfassung:A series of solar radio bursts were observed in AR NOAA 10486 with the Solar Broadband (1.1-7.6 GHz) Radio Spectrometers (SBRS of China). Here we analyze four significant events associated with CME events and strong X-ray flares that occurred on 2003 October 22, 26, 27, 29. The Oct. 26 event is a long duration event (LDE) with drift pulsation structure (DPS), narrowband dm-burst (DCIM), and more than seven types of Fine Structures (FSs); its time of the maximum flux (07:30 UT) is about half an hour later than the X-flare (06:54 UT).
ISSN:1009-9271
DOI:10.1088/1009-9271/4/3/205