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日冕物质抛射与共生射电爆发的地面和空间联测研究 被引量:2

Studies of Coronal Mass Ejections and Associated RadioBursts with the Cooperative Observations of Ground-Basedand Spaceborne Instruments
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摘要 引述了近年来太阳和空间物理的一大研究成果:产生日地空间射电爆发和地球物理响应的主因不是太阳耀斑,而是日冕物质抛射(CME);论述了射电爆发在研究CME中的作用;分析了1991-06-15 CME事件中射电爆发和质子事件产生的物理过程;介绍了地面/空间对 CME和共生射电爆发联测研究的新进展;提出了我国今后开展地面/空间联测研究的设想和建议。 The great achivement in solar-terrestial physics, which the key solar phenomena responsible for interplanetary shocks, non-recurvent geomagnetic storms and large SEPs are caused by the coronal mass ejections (CMEs) instead of flares, is reviewed. The radio signatures of coronal mass ejections are described. The physical processes for the generation of radio bursts and energetic proton streams during the typical event 1991-06-15 CME are discussed in detail, and recent progress in studying the CMEs and associated radio bursts with cooperative observations of ground-based and spaceborne radiospectrograph is presented. Finally, some suggestions for future research works are proposed.
出处 《天文学进展》 CSCD 北大核心 2002年第3期211-222,共12页 Progress In Astronomy
关键词 太阳 日冕物质抛射 射电爆发 激波 磁重联 地球物理响应 sun-CMEs-radio bursts-shock waves-magnetic reconmection-SEPs
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参考文献26

  • 1[1]Kahler S W, Hildner E, Van Hollebeke M A I. Sol. Phys. 1978, 57:429
  • 2[2]Kahler S W et al. J. Geophys. Res. 1984, 89:9683
  • 3[3]Kahler S W et al. Proc. 20th Cosmic Ray. Conf. 1987, 3:121
  • 4[4]Gosling J T. J. Geophys. Res. 1993, 98:18937
  • 5[5]Crooker N U. Nature, 1994, 367:595
  • 6[6]Ryan J M et al. In: Strong K T et al. eds. A Summary of the Results from NASA's Solar Maximum Mission, New York: Springer-Verlag, 1999:457
  • 7[7]Tandberg-Hanssen E, Emslie A G. The Physics of Solar Flares, Lst ed. Cambridge: Cambridge Uni. Press,1988:229
  • 8[9]Reames D V et al. Ap. J. 1997, 491:414
  • 9[10]Fox N J et al. Geophys. Res. Lett. 1998, 25:2461
  • 10[11]Webb D F et al. Geophys. Res. Lett. 1998, 25:2469

同被引文献10

  • 1孙伟英,吴季.太阳宁静及耀斑期间1AU附近等离子体轫致辐射研究[J].空间科学学报,2004,24(6):412-420. 被引量:1
  • 2Gopalswamy N. Coronal mass ejections: Initiation and detection. Adv. Space Res., 2003, 31(4):869-881.
  • 3Kaplan S A, Tsytovich V N. Plasma Astrophysics. Oxford and New York: Pergamon, 1973.
  • 4Bekefi G. Radiation Processes in Plasmas. New York:Wiley, 1966.
  • 5Rybicki G B, Lightman A P. Radiative Processes in Astrophysics. New York: John Wiley and Sons, 1979, 30-35.
  • 6Xie Ruixiang, Wang Min, Yan Yihua, Duan Changchun.Preliminary analysis of a joint observation of the complex solar radio burst of 1998 September 23. Chin. Astron. Astrophys., 2002, 26(3):308-319.
  • 7Babcock R R, Pareer J T. Spectral characteristics of solar radio bursts associated with shortwave fadeouts. J.Atmos. Terr. Phys., 1975, 37(9): 1227-1230.
  • 8Kivelson M G, Russell C T. Intraduction to Space Physics. Cambridge: Cambridge University Press, 1995.
  • 9汪敏,傅其骏,谢瑞祥.太阳微波尖峰辐射的高时间、高频率分辨率偏振观测[J].天体物理学报,2000,20(2):179-188. 被引量:3
  • 10Cheng-Ming Tan,Qi-Jun Fu,Yi-Hua Yan,Yu-Ying Liu National Astronomical Observatories Chinese Academy of Sciences Beijing 100012.Solar Radio Bursts in the Period Oct. 22-Nov. 4, 2003[J].Chinese Journal of Astronomy and Astrophysics,2004,4(3):205-208. 被引量:1

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