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太阳耀斑大气动力学及其光谱诊断 被引量:1

Dynamics of Solar Flare Atmosphere and its Spectral Diagnostics
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摘要 七十年代以来的空间和地面观测表明,太阳耀斑是太阳大气中最剧烈的动力学过程。耀斑动力学的研究已成为当今太阳物理研究中重要的前沿课题之一.本文概要地介绍近年来在耀斑动力学过程的观测和理论方面的重要进展以及耀斑大气动力学的光谱诊断方法,并讨论了今后在观测和理论两方面的努力方向,为我国在即将到来的太阳22周峰年中的耀斑动力学研究提供参考. It has been shown from space and grand-based observations which have been made since 1970's that solar flares are the most violent dynamic process in the solar atmosphere. The study of flare dynamics has already becomes one of the most important frontiers in solar physics. In this paper we present briefly the important progress in observations and theoretical study of flare dynamics in recent years, as well as the spectral diagnostics of flare atmosphere dynamics. Future efforts in both observational and theoretical aspects have also been discussed. This may be taken as a reference for the study of flare dynamics in the coming No. 22 solar cycle.
作者 方成 甘为群
出处 《天文学进展》 CSCD 北大核心 1989年第2期81-90,共10页 Progress In Astronomy
基金 国家自然科学基金 教委博士点资助
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参考文献4

  • 1甘为群,方成.耀斑脉冲相半经验模型[J]空间科学学报,1988(01).
  • 2Gan Wei-Qun,Fang Cheng. Time-match semi-empirical models of the chromospheric flare on 3 February, 1983[J] 1987,Solar Physics(2):311~321
  • 3K. Ichimoto,H. Kurokawa. Hα red asymmetry of solar flares[J] 1984,Solar Physics(1):105~121
  • 4Eijiro Hiei,Kenneth G. Widing. A single loop of 21 January 1974 flare[J] 1979,Solar Physics(2):407~417

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