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Geomagnetic storm,Magnetopause motion,Magnetopause crossing,Plasmasphere dynamics,Geomagnetic field line resonances,Ionospheric currents,IRI UP method,Total electron content
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https://doi.org/10.1186/s40623-019-1056-0
Springer Berlin Heidelberg
Earth, Planets and Space, https://doi.org/10.1186/s40623-019-1056-0
Geomagnetic storm
Magnetopause motion
Magnetopause crossing
Plasmasphere dynamics
Geomagnetic field line resonances
Ionospheric currents
IRI UP method
Total electron content
On some features characterizing the plasmasphere–magnetosphere–ionosphere system during the geomagnetic storm of 27 May 2017
Michael Pezzopane
Afredo Del Corpo
Mirko Piersanti
Claudio Cesaroni
Alessio Pignalberi
Simone Di Matteo
Luca Spogli
Massimo Vellante
Balazs Heilig
10.1186/s40623-019-1056-0
2010-04-23
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Michael Pezzopane
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Afredo Del Corpo
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Mirko Piersanti
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Claudio Cesaroni
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Alessio Pignalberi
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Simone Di Matteo
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Luca Spogli
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Massimo Vellante
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Balazs Heilig
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