首页> 外文会议>The 10th European Solar Physics Meeting Vol.1 Sep 9-14, 2002 Prague, Czech Republic >AN ANALYSIS OP THE SPATIAL FEATURES OF DRIFTING BURSTS IN THE MICROWAVE RANGE
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AN ANALYSIS OP THE SPATIAL FEATURES OF DRIFTING BURSTS IN THE MICROWAVE RANGE

机译:微波范围内爆发爆发的空间特征分析

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摘要

Observations of microwave subsecond pulses (SSP) with high temporal, spatial, and spectral resolution are analyzed. The 30 September 2001 flare with rich fine structure is discussed in detail. For several tens of the SSP drift velocities and positions of the sources are determined. Is shown, that the displacements of sources with a frequency drift on 80 MHz reach a few arcseconds. The irregular character of displacements specifies the presence of plasma density disturbances in the region of the fine structure generation.
机译:分析了具有高时间,空间和光谱分辨率的微波亚秒脉冲(SSP)的观测结果。详细讨论了2001年9月30日火炬,火炬结构丰富。对于几十个SSP,确定了源的漂移速度和位置。如图所示,频率漂移为80 MHz的光源的位移达到几弧秒。位移的不规则特性表明在精细结构产生的区域中存在等离子体密度扰动。

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