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In this paper we will examine ionospheric Joule heating during magnetic storms using global MHD simulations of the interaction of the solar wind with the magnetosphere.
In this work, we examine convection during very strong driving during magnetic storms using global MHD simulations of the interaction of the solar wind with the terrestrial magnetosphere.
In this paper, we will examine the variation of the polar cap potential during magnetic storms using global magnetohydrodynamic (MHD) simulations of the interaction of the solar wind with the magnetosphere.
Fig. 6 Superposed epoch analysis of Dst index and trough position for the four categories of magnetic storms using the normalized time line.
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In this paper, we examine ring current formation during a magnetic storm using global magnetohydrodynamic simulations of the interaction between the solar wind and the magnetosphere.
Furthermore, we have also checked for a direct relationship between the occurrence of flares and E layer density enhancement, during the magnetic storm, using fbEs as a proxy of foE.
The forecasting of magnetic storms by using a moving gradient of the SYM-H index (the symmetric portion of the horizontal component of the magnetic field) as a detecting algorithm has been pointed out by Khabarova et al. (2006).
Analysis of the SYM-H profile of the March 13 14 , 1989super magnetic storm was used to illustrate this point.
Temporal variations of the radiation belt particle during the magnetic storms are investigated using measurements by the low altitude satellite spectrometer.
We study the global properties of energetic (>30 keV) particles during the main and early recovery phase of a major magnetic storm of March 31 , 2001 using data of the NOAA 15 and 16 and the CLUSTER satellites.
For example, Kataoka (2013) has estimated the probability of an extreme magnetic storm comparable in magnitude to the Carrington event occurring in the next decade by using the records of magnetic storms observed at Kakioka.
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