About Geomagnetic energy storage decline
The solar wind-magnetosphere energy transfer is one major way of quantifying the impacts of space weather on the Earth's environment. Studies on solar wind-magnetosphere energy transfer in terms of sub-daily ti.
••A synchrony exists between input and dissipated energy during s.
Interplanetary Coronal Mass Ejections (ICMEs) are the major drivers of space weather events (Gonzalez and Tsurutani, 1987, Gonzalez et al., 1994, Mulligan et al., 1998, Yermolaev.
A total of 85 major geomagnetic storms (Dst≤-100nT) in solar cycle 23 (1996–2006) were identified according to the categorization defined by Gonzalez et al. (1994). We invest.
Table 1 shows the observed distribution of the major geomagnetic storms used in this investigation, based on their interplanetary drivers. The highest occurrence frequency was observed at.
The study of the connections between the strength of a geomagnetic storm and the intrinsic solar stream pressure gained popularity after the famous study by Akasofu and Cha.Therefore, the main thrust of this study is to unveil the energy transfer features of the solar wind-magnetosphere system based on sub-daily time dependence during major geomagnetic storms of solar cycle 23.
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