Revised <I>D<sub>st</sub></I> and the epicycles of magnetic disturbance: 1958–2007
A revised version of the storm-time disturbance index <I>D<sub>st</sub></I> is calculated using hourly-mean magnetic-observatory data from four standard observatories and collected over the years 1958–2007. The calculation algorithm is a revision of that established by Sug...
Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
Copernicus Publications
2009-08-01
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Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/27/3101/2009/angeo-27-3101-2009.pdf |
Summary: | A revised version of the storm-time disturbance index <I>D<sub>st</sub></I> is calculated
using hourly-mean magnetic-observatory data from four standard observatories
and collected over the years 1958–2007. The calculation algorithm is a
revision of that established by Sugiura et al., and which is now used by the
Kyoto World Data Center for routine production of <I>D<sub>st</sub></I>. The most important
new development is for the removal of solar-quiet variation. This is done
through time and frequency-domain band-stop filtering – selectively removing
specific Fourier terms approximating stationary periodic variation driven by
the Earth's rotation, the Moon's orbit, the Earth's orbit around the Sun, and
their mutual coupling. The resulting non-stationary disturbance time series
are weighted by observatory-site geomagnetic latitude and then averaged
together across longitudes to give what we call <I>D<sub>st</sub></I><sup>5807-4SH</sup>. Comparisons are made with the standard Kyoto <I>D<sub>st</sub></I>. Various
biases, especially for residual solar-quiet variation, are identified in the
Kyoto <I>D<sub>st</sub></I>, and occasional storm-time errors in the Kyoto <I>D<sub>st</sub></I> are noted.
Using <I>D<sub>st</sub></I><sup>5807-4SH</sup>, storms are ranked for maximum
storm-time intensity, and we show that storm-occurrence frequency follows a
power-law distribution with an exponential cutoff. The epicycles of magnetic
disturbance are explored: we (1) map low-latitude local-time disturbance
asymmetry, (2) confirm the 27-day storm-recurrence phenomenon using
autocorrelation, (3) investigate the coupled semi-annual-diurnal variation of
magnetic activity and the proposed explanatory equinoctial and
Russell-McPherron hypotheses, and (4) illustrate the well-known solar-cycle
modulation of storm-occurrence likelihood. Since <I>D<sub>st</sub></I><sup>5807-4SH</sup> is useful for a variety of space physics and solid-Earth
applications, it is made freely available to the scientific community. |
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ISSN: | 0992-7689 1432-0576 |