Statistical Study of Geomagnetic Storms during Year 1996-2007

Article Preview

Abstract:

A geomagnetic storm is a global disturbance in Earth’s magnetic field usually occurred due to abnormal conditions in the interplanetary magnetic field (IMF) and solar wind plasma emissions caused by various solar phenomenon. A study of 220 geomagnetic storms associated with disturbance storm time (Dst) decreases of more than -50 nT to -300 nT, observed during 1996-2007, the span of solar cycle 23. We have analyzed and studied them statistically. We find yearly occurrences of geomagnetic storm are strongly correlated with 11-year sunspot cycle, but no significant correlation between the maximum and minimum phase of solar cycle-23 have been found. It is also found that solar cycle-23 is remarkable for occurrence of Intense geomagnetic storm during its declining phase. The detailed results are discussed in this paper.

You might also be interested in these eBooks

Info:

Periodical:

Advanced Materials Research (Volumes 433-440)

Pages:

268-271

Citation:

Online since:

January 2012

Export:

Price:

Permissions CCC:

Permissions PLS:

Сopyright:

© 2012 Trans Tech Publications Ltd. All Rights Reserved

Share:

Citation:

[1] S. I. Akasofu, Solar-wind disturbances and the solar wind-magnetosphere energy coupling function, Space Sci. Rev., 34, 173-183, (1983).

DOI: 10.1007/bf00194625

Google Scholar

[2] W. D. Gonzlez, B. T. Tsurutani, A. L. Clua De Gonzalez, E. J. Smith, F. Tang, S. I. Akasofu, Solar wind Magnetosphere Coupling during Intense Geomagnetic Storms (1978-1979), J. Geophys. Res., 94, 8835-8851, (1989).

DOI: 10.1029/ja094ia07p08835

Google Scholar

[3] Sabbah, The role of interplanetary magnetic field and solar wind in modulating both galactic cosmic rays and geomagnetic activity, Geophys. Res., Lett., 27, 13, (2000).

DOI: 10.1029/2000gl003760

Google Scholar

[4] G. Zhang and L.F. Burlaga, Magnetic clouds geomagnetic disturbances, and cosmic ray decreases, J. Geophys. Res., 93, 2511, (1988).

DOI: 10.1029/ja093ia04p02511

Google Scholar

[5] W. D. Gonzalez, J. A. Joselyn, Y. Kamide, H. W. Kroehl, G. Rostoker, B. T. Tsurutani, V. M. Vasyliunas, What is A Geomagmetic Storm?, J. Geophys. Res., 99, 5771-5792, (1994).

DOI: 10.1029/93ja02867

Google Scholar

[6] R. A. Howard, N. R. Sheeley Jr., M. J. Koomen and D. J. Michels, Coronal Mass Ejections, 1979-1981, J. Geophys. Res., 90, 8173-8191, (1985).

DOI: 10.1029/ja090ia09p08173

Google Scholar

[7] D. F. Webb and R. A. Howard, The solar cycle variation of coronal mass ejections and the solar wind mass flux, J. Geophys. Res., 99, 4201, (1994).

DOI: 10.1029/93ja02742

Google Scholar

[8] J. A. Joselyn and P. S. McIntosh, Disappearing solar filaments: A useful predictor of geomagnetic activity, J. Geophys. Res., 86, 4555, (1981).

DOI: 10.1029/ja086ia06p04555

Google Scholar

[9] C. A. Loewe and G.W. Prolss, Classification and mean behavior of magnetic storms, J. Geophys. Res. 102, 14209, (1997).

Google Scholar

[10] D. A. Couzens and J. H. King, Interplanetary Medium Data Book, NSSDS, WDC-A, Maryland, Suppl. 3, (1986).

Google Scholar

[11] J. H. King, Interplanetary Medium Data Book, NSSDS, WDC-A, Maryland, (1997).

Google Scholar