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Chapman, S. C.; Horne, R. B. and Watkins, N. W.
(2020).
DOI: https://doi.org/10.1029/2019gl086524
Abstract
Geomagnetic indices are routinely used to characterize space weather event intensity. The DST index is well resolved, but is only available over 5 solar cycles. The aa index extends over 14 cycles but is highly discretized with poorly resolved extremes. We parameterize extreme aa activity by the annual averaged top few % of observed values, show these are exponentially distributed and they track annual DST index minima. This gives a 14 cycle average of ~ 4% chance of at least one great (DST<‐500 nT) storm and ~ 28% chance of at least one severe (DST<‐250 nT) storm per year. At least one DST=‐809 [‐663,‐955] nT event in a given year would be a 1:151 year event. Carrington event estimate DST ~ ‐850 nT is within the same distribution as other extreme activity seen in aa since 1868 so that its likelihood can be deduced from that of more moderate events. Events with DST ≲ ‐1000 nT are in a distinct class, requiring special conditions.
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- Item ORO ID
- 69242
- Item Type
- Journal Item
- ISSN
- 1944-8007
- Keywords
- space weather; aa index; Carrington event; geomagnetic storm
- Academic Unit or School
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Faculty of Science, Technology, Engineering and Mathematics (STEM) > Engineering and Innovation
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Copyright Holders
- © 2020 The Authors
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