Solar wind variability and geomagnetic activity
1Department of Physics, Govt. College, Nainpur, District Mandala , M.P. India
2Department of Physics, Govt. College, Beohari, District Shahdol , M.P. India
3Department of Physics, Govt. P.G. Science College, Rewa, , M.P. India
Email:-pankaj_in_2001@rediffmail.com
Solar wind is a dominant feature in interplanetary space at 1AU. In the present analysis, events of high speed solar wind streams (HSSWS) have been taken to derive their relationship with geomagnetic activity for the period of 1996 to 2007; covering the solar cycle 23. Results of present analysis indicate that HSSW streams produce larger geomagnetic field variation during the decreasing phase of solar cycle 23. Minimum solar activity years show smaller increase in Ap values.
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Surendra K. Khandayat1, Gopal Dhurve2 and Pankaj K. Shrivastava3 , "Solar wind variability and geomagnetic activity ", Journal of Ultra Scientist of Physical Sciences, Volume 23, Issue 2, Page Number 494-500, 2016Copy the following to cite this URL:
Surendra K. Khandayat1, Gopal Dhurve2 and Pankaj K. Shrivastava3 , "Solar wind variability and geomagnetic activity ", Journal of Ultra Scientist of Physical Sciences, Volume 23, Issue 2, Page Number 494-500, 2016Available from: http://ultraphysicalsciences.org/paper/642/
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