| Solar Radio Bursts in the Period Oct. 22-Nov. 4, 2003 |
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| 作者姓名： | Cheng-Ming Tan Qi-Jun Fu Yi-Hua Yan Yu-Ying Liu National Astronomical Observatories Chinese Academy of Sciences Beijing |
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| 基金项目： | Supported by the National Natural Science Foundation of China |
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| 摘 要： | A series of solar radio bursts were observed in AR NOAA 10486 withthe Solar Broadband (1.1--7.6 GHz) Radio Spectrometers (SBRS of China). Here weanalyze four significant events associated with CME events and strong X-ray flaresthat occurred on 2003 October 22, 26, 27, 29. The Oct. 26 event is a long durationevent (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).
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| 关 键 词： | 脉冲 无线电 微细结构 分光计 X射线 宽带 窄带 太阳活动周期 |
Solar Radio Bursts in the Period Oct.22-Nov.4, 2003 |
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| Cheng-Ming Tan,Qi-Jun Fu,Yi-Hua Yan,Yu-Ying Liu National Astronomical Observatories Chinese Academy of Sciences Beijing .Solar Radio Bursts in the Period Oct. 22-Nov. 4, 2003[J].Chinese Journal of Astronomy and Astrophysics,2004,4(3):205-208. |
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| Authors: | Cheng-MingTan Qi-JunFu Yi-HuaYan Yu-YingLiu |
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| Institution: | NationalAstronomicalObservatories,ChineseAcademyofSciences,Beijing100012 |
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| Abstract: | 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). |
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| Keywords: | Sun:flares Sun:radio radiation Sun:fine structures |
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