Wavelet Decomposition of Submillimeter Solar Radio Bursts

V.S. Makhmutov; J.-P. Raulin; C.G. Giménez de Castro; P. Kaufmann; E. Correia

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Wavelet Decomposition of Submillimeter Solar Radio Bursts

机译：亚毫米太阳射电爆发的小波分解

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We present the results of wavelet decomposition of fast-time structures during four solar flares observed by the Solar Submillimeter-wave Telescope at 212 GHz. The result of the analysis shows (1) observational evidence on the existence of submm-emission time variations in the range from a few tens of millisecond up to few seconds during solar flares, and (2) that when a solar flare is in progress the time scales reduce as the bulk of the emission flux time variations is increasing.

机译：我们提出了在212 GHz的太阳亚毫米波望远镜观测到的四个太阳耀斑期间快速结构的小波分解结果。分析结果表明：（1）太阳耀斑期间亚毫米发射时间变化的观测证据从几十毫秒到几秒不等；（2）太阳耀斑正在进行时，时间尺度随着大量排放通量时间变化的增加而减小。

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《Solar Physics》 |2003年第2期|211-220|共10页
作者
V.S. Makhmutov; J.-P. Raulin; C.G. Giménez de Castro; P. Kaufmann; E. Correia;
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作者单位

Permanent position at Lebedev Physical Institute RAS;

CRAAM Universidade Presbiteriana Mackenzie;

CRAAM Universidade Presbiteriana Mackenzie;

Part time at CSS UNICAMP SP;

Agreement with INPE;

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Wavelet Decomposition of Submillimeter Solar Radio Bursts

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