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- W3200960163 abstract "Geomagnetic storms are disturbances in the Earth’s magnetosphere. Coronal mass ejections (CMEs) and corotating interaction regions (CIRs) are considered as two major sources of geomagnetic disturbances. Here we have studied halo CMEs and, their solar surface sources and associated geomagnetical disturbances from January, 1996 to December, 2007. During the 12-year period of solar cycle-23 SOHO/LASCO detected 396 full halo CMEs. About 60% of these are found to be front side halo CMEs. These front side CMEs are found to produce geomagnetic storms at the Earth. We examine the properties of these CMEs which produce intense geomagnetic storms (DST ≤ -100 nT). The graphical plot between DST index and speed of CME shows a good correlation between them. It is found that front side CMEs associated with flares, which originate close to the central meridian and the southward component of interplanetary magnetic field BZ are the most potential candidates for producing intense geomagnetic storms. Further the occurrence of geomagnetic storms does not vary with the solar cycle and the mass of CMEs is not correlated with the DST index of storm. Our extensive study, based on complete solar cycle 23 data, confirms the results of previous studies." @default.
- W3200960163 created "2021-09-27" @default.
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- W3200960163 date "2021-01-01" @default.
- W3200960163 modified "2023-10-16" @default.
- W3200960163 title "On solar sources of geomagnetic storms of solar cycle 23 and their relation with CMEs" @default.
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- W3200960163 doi "https://doi.org/10.1063/5.0061278" @default.
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