Large Geomagnetic Storms Drives by Solar Wind in Solar Cycle 24

Various solar phenomena cause anomalous circumstances in the interplanetary magnetic field (IMF) and solar wind plasma emissions. These will produce geomagnetic field disturbances for near earth space at 1AU known as geomagnetic storm. A selection of solar magnetic storm for the period (2010-2017) h...

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Veröffentlicht in:	Journal of physics. Conference series 2019-07, Vol.1234 (1), p.12004
Hauptverfasser:	Al-Feadh, Doha, Al-Ramdhan, Wathiq
Format:	Artikel
Sprache:	eng
Schlagworte:	Coronal Mass Ejection Geomagnetic field Geomagnetism Interplanetary magnetic field Magnetic Storm Magnetic storms Magnetism Solar activity Solar cycle Solar magnetic field Solar maximum Solar phenomena Solar wind Storms Sunspots
Online-Zugang:	Volltext
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