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The occurrence rate of magnetospheric‐substorm onsets: Random and periodic substorms

Borovsky, Joseph E., Nemzek, Robert J., Belian, Richard D.·1993·Journal of Geophysical Research: Space Physics

Abstract

Particle‐injection events are monitored on three geosynchronous satellites to determine the occurrences of magnetospheric substorms: for every consecutive pair of substorms found, the time interval Δ t between substorm onsets is determined. In this manner, 1001 values of Δ t are obtained. A statistical analysis of the Δ t values finds that the most‐probable time between substorms onsets is Δ t ≈ 2.75 hours: this is interpreted to be the period between substorms when substorms occur cyclically. The statistical analysis of the Δ t values also finds a random probability for the occurrence of substorms with a mean time between random substorms of about 5 hours: it is speculated that this random occurrence may be caused by a property of the solar wind that varies randomly with an approximately 5‐hour time scale. About 1500 substorms occur per year: about half are periodic and about half occur randomly.

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Metadata

Authors
Borovsky, J. E., Nemzek, R. J., & Belian, R. D.
Venue
Journal of Geophysical Research: Space Physics
Published
1993-03
Volume
98
Issue
A3
Pages
3807-3813
ISSN
0148-0227 (ISSN-L)
OpenAlex
W2169081815
Cited by
242
References
1
FWCI
8.99
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: The occurrence rate of magnetospheric‐substorm onsets: Random and periodic substorms. https://app.cochat.ai/papers/10.1029/92ja02556
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Borovsky, J. E., Nemzek, R. J., & Belian, R. D. (1993). The occurrence rate of magnetospheric‐substorm onsets: Random and periodic substorms. Journal of Geophysical Research: Space Physics. https://doi.org/10.1029/92ja02556

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