位置:成果数据库 > 期刊 > 期刊详情页
日冕中EUV波的研究进展
  • ISSN号:1000-8349
  • 期刊名称:《天文学进展》
  • 时间:0
  • 分类:P182.6[天文地球—天文学]
  • 作者机构:[1]中国科学院云南天文台,昆明云南650011, [2]云南大学物理科学技术学院,昆明云南650031, [3]云南师范大学旅游地理学院,昆明云南650031
  • 相关基金: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)
中文摘要:

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。

英文摘要:

Extreme Ultraviolet(EUV) waves are large-scale disturbances in the corona.They can pass through the whole solar disk in an hour at the speed of hundreds of kilometers per second. The EUV wave was first discovered by Thompson(1998) when the data from theEUV Imaging Telescope(EIT) were studied. So it was originally named EIT wave. It is now generally called EUV wave since its appearance and properties are not dependent on a specific instrument, and ‘EUV' is more appropriate for describing one of its important physical features. The EUV wave usually has a bright broad relatively-diffuse circular wavefront followed by an expanding dimming region.The EUV wave is thought to be the counterpart of the chromospheric Moreton wave in the corona. However, very few observation including both phenomena has been reported.Moreover, observations showed that EUV waves have two components, a faster wave in front and a slower wave following. These all indicate that the EUV wave and the Moreton wave are not the same. Though having been studied for years, the physical nature and the driving mechanism of EUV waves still remain unclear. Solar flares and coronal mass ejections(CMEs) are the two candidates to drive EUV waves. Currently, both theoretical and observational studies suggested that the flare cannot cause EUV wave, while CME is more likely to drive the EUV wave. In addition, whether EUV waves are the wave or the pseudo-wave or the hybrid wave is still unknown.There are five possible mechanisms for explaining EUV waves: fast mode MHD waves,magnetic field lines successively stretching, successive reconnection, current shell, and slow mode wave or solitary wave. The prevailing scenario of explaining the observational characteristics of EUV waves is of the combination of the first two.Take advantage of the high resolution telescope, we are convinced that EUV waves possess two components, which is supported by many observational evidences. However there are still many unsolved problems, and we hope that we can

同期刊论文项目
同项目期刊论文
期刊信息
  • 《天文学进展》
  • 中国科技核心期刊
  • 主管单位:中国科学院
  • 主办单位:中国科学院上海天文台 中国天文学会
  • 主编:沈志强
  • 地址:上海市南丹路80号406
  • 邮编:200030
  • 邮箱:twxjz@shao.ac.cn
  • 电话:021-34775108
  • 国际标准刊号:ISSN:1000-8349
  • 国内统一刊号:ISSN:31-1340/P
  • 邮发代号:4-819
  • 获奖情况:
  • 1996年在第2届上海市优秀科技期刊评比中获得3等奖...,获得2011年上海市新闻出版局组织的期刊审读优秀奖
  • 国内外数据库收录:
  • 日本日本科学技术振兴机构数据库,中国中国科技核心期刊,中国北大核心期刊(2004版),中国北大核心期刊(2008版),中国北大核心期刊(2011版),中国北大核心期刊(2014版),中国北大核心期刊(2000版)
  • 被引量:1404