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On the origin of microwave type U-bursts
Altyntsev, AT; Kuznetsov, AA; Meshalkina, NS; Yan, YH
2003-11-01
发表期刊ASTRONOMY & ASTROPHYSICS
卷号411期号:2页码:263-271
摘要An analysis is made of the observations of U-type cm-bursts recorded simultaneously with high spatial (Siberian solar radio telescope) and spectral resolution (National Astronomical Observatories/Beijing spectropolarimeters). It is shown that the source positions of increasing and decreasing branches of the U-burst coincide within a few arcsec. The suggestion is made that the occurrence of the observed type U-bursts at microwave frequencies is associated with a pressure and density response to rapid heating pulses in flare loops.
关键词Sun : Flares Sun : Activity Sun : Radio Radiation
DOI10.1051/0004-6361:20031273
收录类别SCI
语种英语
WOS记录号WOS:000186536600031
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被引频次:8[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.bao.ac.cn/handle/114a11/8428
专题太阳物理研究部
作者单位1.Russian Acad Sci, Inst Solar Terr Phys, Siberian Branch, ISTP SB RAS, Irkutsk 664033 33, Russia
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
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Altyntsev, AT,Kuznetsov, AA,Meshalkina, NS,et al. On the origin of microwave type U-bursts[J]. ASTRONOMY & ASTROPHYSICS,2003,411(2):263-271.
APA Altyntsev, AT,Kuznetsov, AA,Meshalkina, NS,&Yan, YH.(2003).On the origin of microwave type U-bursts.ASTRONOMY & ASTROPHYSICS,411(2),263-271.
MLA Altyntsev, AT,et al."On the origin of microwave type U-bursts".ASTRONOMY & ASTROPHYSICS 411.2(2003):263-271.
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