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- W1992076802 abstract "Intense geomagnetic storms (Dst<or equal to -100nT) have been associated with interplanetary structures involving large-intensity (B(sub 3)<or equal to 10nT) and long-duration (T< or equal to 3 hours) values of the southward component of the IMF. We show that near solar maximum, the solar origin of such structures seems to be associated with active regions(flares and/or filament eruptions) ocurring close to the streamer belt and to growing low altitude coronal holes. It is also shown that such type of coronal holes had a dual-peak solar cycle distribution during solar cycle 21, similar to that previously reported for the above mentioned interplanetary and geomagnetic phenomena." @default.
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- W1992076802 date "1996-09-15" @default.
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- W1992076802 title "Coronal hole-active region-Current sheet (CHARCS) Association with intense interplanetary and geomagnetic activity" @default.
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- W1992076802 doi "https://doi.org/10.1029/96gl02393" @default.
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