日冕中EUV波的研究进展
发布时间：2018-11-15 14:58
【摘要】：日冕极紫外(EUV)波是Thompson等人1998年首先在EIT的观测资料中发现的,在日冕中以几百km/s的速度传播的扰动现象,在1 h之内扫过了大部分太阳表面,所以这个现象开始被称为"EIT波"。首先介绍了EUV波的研究背景;然后介绍了EUV波的观测特征;第3章分别介绍了EUV波与Moreton波、耀斑及CME的关系;第4章介绍了从发现EUV波以来提出的各种理论和模型;第5章讨论到目前为止已发现的EUV波成分:一个较快的波在前面传播,一个较慢的波在后面传播;最后,对EUV波研究的未来方向及发展趋势进行了总结和展望。
[Abstract]:The coronal extreme ultraviolet (EUV) wave was first discovered by Thompson et al in 1998 in the EIT observation data. The disturbance phenomenon propagating at the speed of several hundred km/s in the corona swept most of the solar surface within one hour. So this phenomenon began to be called EIT waves. The research background of EUV wave is introduced at first, then the observational characteristics of EUV wave are introduced, the relationship between EUV wave and Moreton wave, flare and CME is introduced in chapter 3, and the theories and models since EUV wave are discovered are introduced in chapter 4. Chapter 5 discusses the components of EUV wave which have been found so far: a faster wave propagates in front and a slower wave propagates behind. Finally, the future direction and development trend of EUV wave research are summarized and prospected.
【作者单位】： 中国科学院云南天文台;云南大学物理科学技术学院;云南师范大学旅游地理学院;
【基金】：973项目(2011CB811403,2013CBA01503) 国家基金项目(11273055,11333007) 中国科学院创新工程方向性项目(KJCX2-EW-T07)
【分类号】：P182.62
本文编号：2333622
[Abstract]:The coronal extreme ultraviolet (EUV) wave was first discovered by Thompson et al in 1998 in the EIT observation data. The disturbance phenomenon propagating at the speed of several hundred km/s in the corona swept most of the solar surface within one hour. So this phenomenon began to be called EIT waves. The research background of EUV wave is introduced at first, then the observational characteristics of EUV wave are introduced, the relationship between EUV wave and Moreton wave, flare and CME is introduced in chapter 3, and the theories and models since EUV wave are discovered are introduced in chapter 4. Chapter 5 discusses the components of EUV wave which have been found so far: a faster wave propagates in front and a slower wave propagates behind. Finally, the future direction and development trend of EUV wave research are summarized and prospected.
【作者单位】： 中国科学院云南天文台;云南大学物理科学技术学院;云南师范大学旅游地理学院;
【基金】：973项目(2011CB811403,2013CBA01503) 国家基金项目(11273055,11333007) 中国科学院创新工程方向性项目(KJCX2-EW-T07)
【分类号】：P182.62
【相似文献】
相关期刊论文 前1条
1 黄光力;;1998年11月28日耀斑-CME事件的射电和EUV特征[J];中国科学A辑;2001年S1期
，本文编号：2333622
本文链接：https://www.wllwen.com/kejilunwen/tianwen/2333622.html
