Radio bursts with rapid frequency variations -: Lace bursts

被引:50
作者
Karlicky, M [1 ]
Bárta, M
Jiricka, K
Mészárosová, H
Sawant, HS
Fernandes, FCR
Cecatto, JR
机构
[1] Acad Sci Czech Republ, Inst Astron, CS-25165 Ondrejov, Czech Republic
[2] Inst Nacl Pesquisas Espaciais, BR-12201970 Sao Jose Dos Campos, SP, Brazil
基金
巴西圣保罗研究基金会;
关键词
Sun : activity; Sun : flares; Sun : radio radiation;
D O I
10.1051/0004-6361:20010888
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Ondrejov radiospectrograph operating in the 0.8-2.0 GHz frequency range recorded in recent years (1998-2000), three (August 10, 1998; August 17, 1999; June 27, 2000) unique bursts with rapid frequency variations (lace bursts) lasting for several minutes. On August 17, 1999, the same burst was recorded simultaneously by the Brazilian Solar Spectroscope in the 1.0-2.5 GHz frequency range. The frequency variations of these bursts in four time intervals were analyzed by the Fourier method and power-law spectra with power-law indices close to -2 were found. The Fourier spectra show the presence of frequency variations in the 0.01-3.0 Hz interval which indicate fast changes of plasma parameters in the radio source. Due to the similarities in the line features of these bursts with zebra pattern lines, a model similar to that of the zebra pattern was suggested. The model radio spectra, computed using this model with a turbulent state of the solar are atmosphere, are similar to those observed by the radiospectrographs.
引用
收藏
页码:638 / 642
页数:5
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