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TEMPORAL ANALYSIS OF GEOMAGNETIC STORM INTENSITY: INSIGHTS FROM SOLAR ACTIVITY DATA (1996-2022)
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Author(s):
DR. NAVAL KISHOR LOHANI, PRIYANSHU GUPTA
Vol - 13, Issue- 3 ,
Page(s) : 83 - 92
(2023 )
DOI : https://doi.org/10.32804/RJSET
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Abstract
The acceleration of solar wind remains one of the unsolved fundamental problems in solar physics. The two most important processes which are used to explain the excitation of solar wind are thermal excitation of solar wind and magnetic excitation of solar wind.
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