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Effect of Altitude on the Position of the Magnetic Pole

Abstract

IN the most recent analysis of the Earth's magnetic field (for the epoch 1942), Spencer Jones and Melotte1 evaluated forty-eight coefficients in the spherical harmonic expansion of the magnetic potential. Using their values for a spheroidal Earth, the X (northerly) and Y (easterly) components of the Earth's magnetic field were calculated at heights of 100 km. and 250 km. above the Earth's surface for θ = 5°, 10°, 15°, 20° and 25° and for ϕ = 240°, 250° and 260° E., where θ and ϕ are the co-latitude and longitude respectively. The heights 100 and 250 km. were chosen to correspond to the E- and F-layers of the ionosphere. For the purpose of comparison, X and Y were also evaluated at the Earth's surface and in every case the value of H = (X 2 + Y 2)1,2 was computed.

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References

  1. Spencer Jones, H., and Melotte, P. J., Mon. Not. Roy. Astro. Soc., Geophys. Supp., 6, 409 (1953).

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JACOBS, J. Effect of Altitude on the Position of the Magnetic Pole. Nature 178, 35–36 (1956). https://doi.org/10.1038/178035b0

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  • DOI: https://doi.org/10.1038/178035b0

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