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- W4213309211 abstract "at the equinoxes than near the solstices. The great problem storms of the last four solar cycles, i.e., those storms lacking commensurate preceding solar activity, are all found to occur relatively near the equinoxes. Conversely, four of the five great storms that occurred near the solstices were preceded by truly outstanding solar flares. About half (11/25) of the great storms had obvious precursor geomagnetic activity, i.e., periods of approximately > 1 day with D sub st approximately < {minus}30 nT. The precursors can enable some weaker solar events to be more geoeffective than would otherwise be the case in two ways: (1) compression and amplification of pre-existing southward (precursor) fields by the transient shock, and (2) establishment of a lower D sub st baseline , making it easier for transient events to drive D sub st to values < or = {minus}250 nT." @default.
- W4213309211 created "2022-02-24" @default.
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- W4213309211 creator A5078064076 @default.
- W4213309211 date "2022-02-08" @default.
- W4213309211 modified "2023-09-27" @default.
- W4213309211 title "Toward Forecasting Geomagnetic Storms" @default.
- W4213309211 doi "https://doi.org/10.2172/1845219" @default.
- W4213309211 hasPublicationYear "2022" @default.
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