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Ⅲ型爆发及其在太阳大气行星际等离子体中的传播 被引量:2

Type Iff Burst and Its Propagation in Solar Atmospheric and Interplanetary Plasma
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摘要 本文以近20年来Ⅲ型爆发的地面观测和空间探测的巨大成就,概述了Ⅲ型爆发的主要特征,源的高度、大小以及波的传播效应。它的内向漂移特征,同spike、X射线辐射及其色球耀斑的可能关系,它的外向漂移特征,同行星际磁场线的关系及其对宇宙线的可能调制作用。 Based on the great success of type Ⅲ bursts obtained by ground and space radio observations in recent two decades, we describe important characteristics of type Ⅲ bursts, height and size of radio sources, as well as propagation effects of radio wave in solar atmospheric and interplanetary plasma. Their inward drift in solar atmosphere, which is possibly related to spike, X-ray and flare as well as the outward drift,which might have relation with interplanetary magnetic field line and modulation effect to cosmic rays are discussed in this paper.
出处 《天文学进展》 CSCD 北大核心 1990年第3期179-188,共10页 Progress In Astronomy
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  • 1王震江.太阳磁场和宇宙线实验规律初探[J]天文学进展,1988(02).
  • 2D. B. Melrose. The emission mechanisms for solar radio bursts[J] 1980,Space Science Reviews(1):3~38
  • 3C. Mercier,H. Rosenberg. Type III solar radio bursts observed at 169 MHz: Height and relative positions in pairs[J] 1974,Solar Physics(1):193~206
  • 4H. Alvarez,F. Haddock,R. P. Lin. Evidence for electron excitation of type III radio burst emission[J] 1972,Solar Physics(2):468~473

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