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Drifting radio bursts and fine structures in the 0.8-7.6 GHz frequency range observed in the NOAA 9077 AR (July 10-14, 2000) solar flares
Karlicky, M; Yan, Y; Fu, Q; Wang, S; Jiricka, K; Meszaroscova, H; Liu, Y
2001-04-01
发表期刊ASTRONOMY & ASTROPHYSICS
卷号369期号:3页码:1104-1111
摘要The 0.8-7.6 GHz global and detailed radio spectra of the four most intense flares observed in the NOAA 9077 active region (July 10-14, 2000) are presented. The radio bursts of these flares and their sequence reveal features indicative of topological similarities among the flares under study. The drifting pulsation structures mere found to be the typical signatures of these flares. Furthermore many other fine structures such as narrowband drifting lines, drifting harmonic structure with zebra patterns, drifting branches of narrowband dm-spikes, and structures with fast positively and negatively drifting bursts are shown in the contest of the whole radio flares. Same of them were observed for the first time. The relationships among them and the resulting interpretations ale summarized. The characteristic periods of the drifting pulsation structures and the magnetic field in the zebra radio source are determined.
关键词Sun : Activity Sun : Flares Sun : Radio Radiation
收录类别SCI
语种英语
WOS记录号WOS:000168457800035
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文献类型期刊论文
条目标识符http://ir.bao.ac.cn/handle/114a11/8590
专题太阳物理研究部
作者单位1.Acad Sci Czech Republ, Inst Astron, CS-25165 Ondrejov, Czech Republic
2.Chinese Acad Sci, Natl Astron Observ, Beijing Astron Observ, Beijing 100012, Peoples R China
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Karlicky, M,Yan, Y,Fu, Q,et al. Drifting radio bursts and fine structures in the 0.8-7.6 GHz frequency range observed in the NOAA 9077 AR (July 10-14, 2000) solar flares[J]. ASTRONOMY & ASTROPHYSICS,2001,369(3):1104-1111.
APA Karlicky, M.,Yan, Y.,Fu, Q.,Wang, S.,Jiricka, K.,...&Liu, Y.(2001).Drifting radio bursts and fine structures in the 0.8-7.6 GHz frequency range observed in the NOAA 9077 AR (July 10-14, 2000) solar flares.ASTRONOMY & ASTROPHYSICS,369(3),1104-1111.
MLA Karlicky, M,et al."Drifting radio bursts and fine structures in the 0.8-7.6 GHz frequency range observed in the NOAA 9077 AR (July 10-14, 2000) solar flares".ASTRONOMY & ASTROPHYSICS 369.3(2001):1104-1111.
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