Quasi-linear model for the plasma mechanism of narrow-band microwave burst generation
Quasi-linear model for the plasma mechanism of narrow-band microwave burst generation
复制标题
窄带微波爆发产生等离子体机制的准线性模型
DOI:
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发表时间:
1993
期刊:
影响因子:
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通讯作者:
V. Mel’nikov
中科院分区:
文献类型:
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作者:
B. N. Levin;V. Mel’nikov
Characteristic features of the plasma model for radio emission from the extending fronts of solar flare energy release are studied. It is shown that the electron distribution is formed near the thermal fronts as stationary beam injection through the boundary into the cold plasma semi-space. A principal new result is a conclusion about the localization of a plasma turbulence region — the source of emission in a narrow layer before the thermal front, that makes it possible to explain the burst narrow-band feature in a natural way. Wide capabilities of the flare loop structure analysis using the narrow-band emission parameters are demonstrated.