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Motion of the Earth’s magnetic poles in the last decade

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Abstract

Based on vector magnetic data from the CHAMP German satellite, average daily spherical harmonic models of the main geomagnetic field to n = m = 10 have been constructed for the period from May 2001 to the end of 2009 at an interval of 4 days. The obtained 16 models, which were averaged over half a year, have been used to calculate the coordinates of the north and south magnetic poles (the points where magnetic field lines are vertical). The changes in these coordinates during these eight and a half years have been traced. Both poles continue moving northward and westward. The north magnetic pole has traveled 400 km during this period. The velocity of its motion has increased up to the year 2003, reaching 62.5 km yr−1, and then started decreasing and reached 45 km yr−1 by the end of 2009. In addition, the direction of motion changed from north-northwestward to northwestward; i.e., the pole started turning slightly towards Canada. The south magnetic pole moved slower by an order of magnitude and has traveled 42 km during this period. The coordinates of the geomagnetic (dipole) poles and the eccentric dipole parameters have also been calculated. The dynamics of these poles has been traced.

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Authors and Affiliations

  1. Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation, Russian Academy of Sciences, Troitsk, Moscow oblast, 142190, Russia

    T. I. Zvereva

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  1. T. I. Zvereva
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Correspondence to T. I. Zvereva.

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Original Russian Text © T.I. Zvereva, 2012, published in Geomagnetizm i Aeronomiya, 2012, Vol. 52, No. 2, pp. 278–286.

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Zvereva, T.I. Motion of the Earth’s magnetic poles in the last decade. Geomagn. Aeron. 52, 261–269 (2012). https://doi.org/10.1134/S0016793212020168

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