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Lunar Magnetic Variations

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Quiet Daily Geomagnetic Fields

Part of the book series: Pageoph Topical Volumes ((PTV))

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Abstract

Displayed daygraphs of magnetic observatory hourly mean values and of lunar magnetic variations reconstructed from spherical harmonic coefficients are used to illustrate the difficulties that arise in separating lunar magnetic effects from those associated with the 27 day recurrence tendency in magnetic activity.

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References

  • Malin, S. R. C. (1970), Separation of Lunar Daily Geomagnetic Variations into Parts of Ionospheric and Oceanic Origin, Geophys. J. Roy. Astr. Soc. 21, 447–455.

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  • Stening, R. J., and Winch, D. E. (1987), The Lunar Geomagnetic Tide at Night, Geophys. J. R. Astr. Soc. 88, 461–476.

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  • Winch, D. E. (1981), Spherical Harmonic Analysis of Geomagnetic Tides, 1964–1965, Phil. Trans. R. Soc. Lond. A303, 1–104.

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  • Winch, D. E., and Cunningham, R. A. (1972), Lunar Magnetic Tides at Wath-eroo, Seasonal, Elliptic, Evectional, Variational and Nodal Components, J. Geomag. Geoelect. 24, 381–414.

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© 1989 Birkhäuser Verlag, Basel

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Winch, D.E. (1989). Lunar Magnetic Variations. In: Campbell, W.H. (eds) Quiet Daily Geomagnetic Fields. Pageoph Topical Volumes. Birkhäuser Basel. https://doi.org/10.1007/978-3-0348-9280-3_15

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  • DOI: https://doi.org/10.1007/978-3-0348-9280-3_15

  • Publisher Name: Birkhäuser Basel

  • Print ISBN: 978-3-7643-2338-7

  • Online ISBN: 978-3-0348-9280-3

  • eBook Packages: Springer Book Archive

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