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Comprehensive Studies on Magnetic Clouds in Interplanetary Space and their Associated Events

  • WANG Yu-Ming ,
  • WANG Shui
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  • School of Earth and Space Sciences, University of Science and Technology of Chi na, Hefei 230026, China

Received date: 2004-04-19

  Online published: 2005-03-15

Abstract

The relationships between the coronal mass ejections (CMEs), interplanetary disturbances and geomagnetic storms are studied, involving the solar source distribution of geoeffective halo CMEs, the periodicity of CMEs, X-ray flares and geomagnetic disturbances, the threshold of interplanetary parameters in causing geomagnetic storms, etc. As a kind of interplanetary complex structure, multiple magnetic cloud (Multi-MC) is proposed for the first time, which probably has strong geoeffectiveness.Based on the observations, some primary characteristics of Multi-MC are summarized. Moreover, the phenomenon of a shock advancing into a preceding magnetic cloud has been investigated as well as its potential geoeffectiveness. A simple theoretical model is developed to estimate the intensity of geomagnetic storm when a shock is entering a preceding cloud.

Cite this article

WANG Yu-Ming , WANG Shui . Comprehensive Studies on Magnetic Clouds in Interplanetary Space and their Associated Events[J]. Journal of University of Chinese Academy of Sciences, 2005 , 22(2) : 248 -254 . DOI: 10.7523/j.issn.2095-6134.2005.2.019

References

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[2] Wang YM, Ye PZ, Wang S, et al. A statistical study on the geoeffectiveness of Earth2directed coronal mass ejections from March 1997 toDecember 2000. J. Geophys. Res., 2002, 107 : 1340

[3] Ye PZ, Wang YM. A study on the Bs events in interplanetary space and the associated CMEs in 2002. Chinese J. Space Sci., 2003, 23 : 7~17

[4] Wang YM, Shen CL, Ye PZ, et al. Deflection of coronal mass ejections in the interplanetary medium. Sol. Phys., 2004,222 :329~343

[5] Lou YQ, Wang YM, Fan Z, et al. Periodicities in solar coronal mass ejections. Mon. Not. R. Astron. Soc., 2003, 345 : 809~818

[6] Wang YM, Shen CL, Wang S, et al. An empirical formula relating the geomagnetic storm’s intensity to the interplanetary parameters : 2 VBz andΔt. Geophys. Res. Lett., 2003, 30 : 2039

[7] ang YM, Wang S, Ye PZ. Multiple magnetic clouds in interplanetary space. Sol. Phys., 2002, 211 : 333~344

[8] Wang YM, Ye PZ, Wang S. Multiple magnetic clouds : several examples during March 2 April 2001. J. Geophys. Res., 2003, 108 : 1370

[9] Wang YM, Ye PZ, Wang S. A probable origin of great geomagnetic storm: multiple magnetic clouds. Chinese J. Geophys., 2004,47 :417~423

[10] Wang YM, Zheng HN, Wang S. MHD simulation of the formation and propagation of multiple magnetic clouds in the heliosphere. Astron. andAstrophys, 2004 (in Press)

[11] Wang YM, Ye PZ, Wang S, et al, An interplanetary cause of large geomagnetic storms : Fast forward shock overtaking preceding magnetic cloud.Geophys. Res. Lett., 2003, 30 :1700

[12] Wang YM, Ye PZ, Wang S, et al. Theoretical analysis on the geoeffectiveness of shock overtaking preceding magnetic cloud. Sol. Phys, 2003,216 : 295~310

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