Abstract

Abstract. A previous application of extreme-value statistics to the first, second and third largest geomagnetic storms per solar cycle for nine solar cycles is extended to fourteen solar cycles (1844–1993). The intensity of a geomagnetic storm is measured by the magnitude of the daily aa index, rather than the half-daily aa index used previously. Values of the conventional aa index (1868–1993), supplemented by the Helsinki Ak index (1844–1880), provide an almost continuous, and largely homogeneous, daily measure of geomagnetic activity over an interval of 150 years. As in the earlier investigation, analytic expressions giving the probabilities of the three greatest storms (extreme values) per solar cycle, as continuous functions of storm magnitude (aa), are obtained by least-squares fitting of the observations to the appropriate theoretical extreme-value probability functions. These expressions are used to obtain the statistical characteristics of the extreme values; namely, the mode, median, mean, standard deviation and relative dispersion. Since the Ak index may not provide an entirely homogeneous extension of the aa index, the statistical analysis is performed separately for twelve solar cycles (1868–1993), as well as nine solar cycles (1868–1967). The results are utilized to determine the expected ranges of the extreme values as a function of the number of solar cycles. For fourteen solar cycles, the expected ranges of the daily aa index for the first, second and third largest geomagnetic storms per solar cycle decrease monotonically in magnitude, contrary to the situation for the half-daily aa index over nine solar cycles. The observed range of the first extreme daily aa index for fourteen solar cycles is 159–352 nT and for twelve solar cycles is 215–352 nT. In a group of 100 solar cycles the expected ranges are expanded to 137–539 and 177–511 nT, which represent increases of 108% and 144% in the respective ranges. Thus there is at least a 99% probability that the daily aa index will satisfy the condition aa < 550 for the largest geomagnetic storm in the next 100 solar cycles. The statistical analysis is used to infer that remarkable conjugate auroral observations on the night of 16 September 1770, which were recorded during the first voyage of Captain Cook to Australia, occurred during an intense geomagnetic storm.

Highlights

  • Siscoe (1976) applied the statistics of extremes to the®rst, second and third largest geomagnetic storms in nine solar cycles, as measured by the average half-daily aa index

  • Results for solar cycles 9 to 22 involve the inclusion of two additional solar cycles prior to 1868, which requires the use of the Helsinki Ak index

  • The daily Ak index is intended to provide an extension of the daily aa index backwards in time to 1844 (Nevanlinna and Kataja, 1993), it may not provide a completely homogeneous extension of this latter index

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Summary

Introduction

®rst, second and third largest geomagnetic storms in nine solar cycles (viz. 11 to 19), as measured by the average half-daily aa index. ®rst, second and third largest geomagnetic storms in nine solar cycles The conventional daily aa index (Mayaud, 1980) is available electronically through the National Geophysical Data Center, Boulder, Colorado, for the interval 1868±1993, which extends by almost three solar cycles the time-interval considered by Siscoe. Values of the`essentially equivalent'' Helsinki magnetic activity index Ak are available electronically through the Finnish Meteorological Institute, Helsinki (Nevanlinna, 1995). ®rst, second and third largest geomagnetic storms per solar cycle over a 150-year interval (1844±1993), using essentially homogeneous daily values of the aa index of geomagnetic activity. It is important to consider all three cases separately because there are 137 missing daily values of the Ak index in the interval 1844±1867, which might just possibly inuence the results for fourteen solar cycles.

Derivation of the aa and Ak indices
Attributes and limitations of the extended aa index
Application of the statistics of extremes to geomagnetic storms
Statistical characteristics of the extreme values
Probabilities of the three largest geomagnetic storms per solar cycle
The expected ranges of extreme storms for a given number of solar cycles
Conclusions and discussion
10 S of the equator between Timor and the island of
April 1858 produced an aurora that was visible from
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