期刊文献+

2012年1月23日SEP事件的“twin-CME”爆发现象 被引量:1

The Compound “twin-CME” Eruptions Associated with Extreme SEP Event on January 23,2012
下载PDF
导出
摘要 "twin-CME"模型是Li等人提出的一种比单个CME更高效的产生SEP事件的模型。本文主要以"twin-CME"模型为出发点,综合运用SOHO/LASCO、STEREO-A/SECCHI、STEREO-B/SECCHI的日冕观测及CME的GCS模拟,Learmonth、BIRS和Wind/WAVES射电观测,以及SDO/AIA源区观测和SDO/HMI磁图资料,分析2012年1月23日爆发的极端SEP事件的源区爆发特征。结果表明:此SEP事件对应的源区观测到"twin-CME"爆发,即从同一源区先后相继爆发了2个CME,这2个CME在空间的传播方向基本一致,并在传播到一定高度时发生相互作用合并成一个更强的CME,此爆发过程CME和源区磁场特征与"twin-CME"模型的假设基本相似。"twin-CME"爆发及双CME合并可能是引起此极端SEP事件的原因。 The"twin-CME"scenario proposed by Li et al.(2012)which can produce large solar energetic particle(SEP)event more efficiently than the"Single-CME".Based on"twin-CME"scenario in this paper,spatial characteristics of CME eruptions associated with January 23 2012 extreme SEP event were analyzed,using CME observations detected by coronagraph instruments onboard SOHO/LASCO and STEREO-A(B)/SECCHI,fitting for CME by GCS model.In this event,the process of CMEs erupting from their source region was checked in low corona,such as the association of typeⅡ radio bursts detected by Learmonth and BIRS ground stations Wind/WAVES instruments,the associated AIA multiwaveband images on board SDO spacecraft,and HMI magnetogram.The results show that there are two successive CME eruptions associated with this SEP event.These two CMEs have similar propagation direction,and can merge into one large strong CME after certain period of time.The topology of magnetic polarity and eruption process of source region is similar to that of"twin-CME"scenario.The"twin-CME"eruption and the two CMEs mergence may be responsible for generating this extreme large SEP event.
出处 《广西师范大学学报(自然科学版)》 CAS 北大核心 2014年第3期12-21,共10页 Journal of Guangxi Normal University:Natural Science Edition
基金 国家自然科学基金资助项目(41304150 41174165) 江苏省高校自然科学基金项目(12KJB170008)
关键词 太阳高能粒子 日冕物质抛射 双CME 空间天气 solar energetic particle coronal mass ejection twin-CME space weather
  • 相关文献

参考文献24

  • 1REAMES D V. Particle acceleration at the Sun and in the heliosphere[J]. Space Sci Rev, 1999, 90:413-491.
  • 2KAHLER S W. Coronal mass ejections and solar energetic particle events[J]. AIP Conference Proceedings, 1996, 374 (1) :61-77.
  • 3KAHLER S W. The correlation between solar energetic particle peak intensities and speeds of coronal mass ejections= Effects of ambient particle intensities and energy spectra[J]. Journal of Geophysical Research, 2001, 106(A10): 20947-20955.
  • 4PAN Z H, WANG Chuan bing, WANG Y, et al. Correlation Analyses Between the Characteristic Times of Gradual Solar Energetic Particle Events and the Properties of Associated Coronal Mass Ejections[J]. Solar Physics, 2011, 270 (2) :593-607.
  • 5KAHLER S W, REAMES D V, BURKEPIL[J T. A role for ambient energetic particle intensities in shock accelera- tion of solar energetic particles[J]. ASP Conference, 2000, 206:468-468.
  • 6MASON G M, MAZUR J E, DWYER J R. *3He enhancements in large solar energetic particle events[J]. AstroPhys,1999, 525:L133-L136.
  • 7GOPALSWAMY N, YASHIRO S, KRUCKER S, et al. Intensity variation o{ large solar energetic particle events as- sociated with coronal mass ejections[J]. Journal of Geophysical Research, 2004, 109(A12) :lq8.
  • 8DING Liu-guan, YONG Jiang, ZHAO Lu]u, et al. The "Twin-Cme" scenario and large solar energetic particle events in solar cycle 23[J]. The Astrophysical Journal, 2013, 763(1) :30-30.
  • 9LI Gang, MOORE R, MEWALDT R A, et al. A twin CME scenario for ground level enhancement events[J]. Space Science Reviews, 2012, 171(1-4):141 160.
  • 10LI Gang, ZANK G. Multiple CMEs and large gradual SEP eventsC//29th ICRC Proceedings. Mumbai: Tara Insti- tute of Fundamental Research, 2005, 1 : 173 173.

二级参考文献93

  • 1Reames D V, Space Science Reviews, 1999, 90(3): 413.
  • 2Gonzalez W, Joselyn J, Kamide Y, et al. Journal of Geophysical Research, 1994, 99(A4): 5771.
  • 3Zhang J, Dere K P, Howard R A, et al. Astrophysical Journal, 2003, 582(1): 520.
  • 4Gui B, Shen C, Wang Y, et al. Solar Physics, 2011, 271: 111.
  • 5Shen C, Wang Y, Gui B, et al. Solar Physics, 2011, 269(2): 389.
  • 6Wei F, Dryer M. Solar Physics (ISSN 0038-0938), 1991, 132:373.
  • 7Zuccarello F P, Bemporad A, Jacobs C, et al. Astrophysical Journal, 2012, 744(1): 66.
  • 8Wiegelmann T, Sakurai T. Living Reviews in Solar Physics, 2012, 9:5.
  • 9Jiang C, Feng X, Wu S T, et al. Astrophysical Journal, 2012, 759(2): 85.
  • 10Jiang C, Feng X, Xiang C. Astrophysical Journal, 2012, 755(1): 62.

共引文献3

引证文献1

二级引证文献5

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部