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Correct Normalization of the Dst Index : Volume 4, Issue 2 (18/07/2008)

By Mursula, K.

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Book Id: WPLBN0003991989
Format Type: PDF Article :
File Size: Pages 5
Reproduction Date: 2015

Title: Correct Normalization of the Dst Index : Volume 4, Issue 2 (18/07/2008)  
Author: Mursula, K.
Volume: Vol. 4, Issue 2
Language: English
Subject: Science, Astrophysics, Space
Collections: Periodicals: Journal and Magazine Collection, Copernicus GmbH
Historic
Publication Date:
2008
Publisher: Copernicus Gmbh, Göttingen, Germany
Member Page: Copernicus Publications

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Holappa, L., Karinen, A., & Mursula, K. (2008). Correct Normalization of the Dst Index : Volume 4, Issue 2 (18/07/2008). Retrieved from http://hawaiilibrary.net/


Description
Description: Department of Physical Sciences, P.O.Box 3000, FIN-90014, University of Oulu, Finland. The Dst index has been one of the most important solar-terrestrial indices for decades, and it is used in numerous studies as a measure of the temporal development and intensity of magnetic storms and the ring current. Here we discuss two issues related to the relative and absolute normalization that are problematic to the Dst index. We show for the first time quantitatively that the magnetic disturbances at the four Dst stations are ordered according to the latitudinal projection of an equatorial disturbance upon the local horizontal component of the geomagnetic field. Therefore, the disturbances observed at each station should be first normalized by the cosine of the geomagnetic latitude of the station before they are averaged to form the Dst index. Perhaps surprisingly, the recipe to calculate the Dst index does not include this normalization and, therefore, must be revised on this part. We also discuss the effects of correcting the quiet-time seasonal variation, the so called non-storm component in the Dst index. This correction is seasonally varying, being largest around equinoxes and smallest at solstices, leading to an average correction (increase) of about 6 nT, i.e. about 25–30%, for annual averages of the Dst index. This increase also leads to significantly improved correlations between the corrected Dst index, the so called Dcx index, and many other indices of solar-terrestrial disturbance. We show here in detail that the correlation between the geomagnetic Ap index and the Dcx index (cc = 0.83) is much higher than between Ap and Dst (cc = 0.60). These results give further evidence that the Dcx index is a more truthful measure of magnetic storminess than the original Dst index.

Summary
Correct normalization of the Dst index

Excerpt
Cliver, E. W., Kamide,~Y., Ling,~A G., and Yokoyama,~N.: Semiannual variation of the geomagnetic \emphDst index: Evidence for a dominant nonstorm component, J. Geophys. Res., 106, 21 297–21 304, 2001.; Karinen, A. and Mursula,~K.: A new reconstruction of the \emphDst index for 1932–2002, Ann. Geophys., 23, 475–485, 2005.; Karinen, A. and Mursula,~K.: Correcting the \emphDst index: Consequences for absolute level and correlations, J. Geophys. Res., 111, A08207, doi:10.1029/2005JA011299, 2006.; Mursula, K. and Karinen,~A.: Explaining and correcting the excessive semiannual variation in the \emphDst index, Geophys. Res. Lett., 32, L14107, doi:10.1029/2005GL023132, 2005.; Sugiura, M.: IAGA Resolution 2, in IAGA Bulletin, Madrid, Spain, 27, 123, 1969.; Sugiura, M. and Kamei,~T.: Equatorial \emphDst index 1957–1986, in IAGA Bull., 40, edited by A. Berthelier and M. Menvielle, ISGI Publ. Off., Saint-Maur-des-Fossés, France, 1991.; WDC-C2, Definition of the \emphDst index. The World Data Center for Geomagnetism (WDC-C2), http://swdcdb.kugi.kyoto-u.ac.jp, Kyoto, Japan, 2004.

 

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