Statistics of the largest geomagnetic storms per solar cycle (1844-1993)
Item
Title (Dublin Core)
Statistics of the largest geomagnetic storms per solar cycle (1844-1993)
Description (Dublin Core)
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 <i>aa</i> index, rather than the half-daily <i>aa</i> index used previously. Values of the conventional <i>aa</i> index (1868–1993), supplemented by the Helsinki <i>Ak</i> 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 (<i>aa</i>), 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 <i>Ak</i> index may not provide an entirely homogeneous extension of the <i>aa</i> 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 <i>aa</i> 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 <i>aa</i> index over nine solar cycles. The observed range of the first extreme daily <i>aa</i> 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 <i>aa</i> index will satisfy the condition <i>aa</i> < 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.
Creator (Dublin Core)
Willis, D. M.
Stevens, P. R.
Crothers, S. R.
Date (Dublin Core)
2018-09-27
Type (Dublin Core)
Text
Format (Dublin Core)
application/pdf
Identifier (Dublin Core)
10.1007/s00585-997-0719-5
https://angeo.copernicus.org/articles/15/719/1997/
Source (Dublin Core)
eISSN: 1432-0576
Language (Dublin Core)
eng



