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The Spectrum of the Magnetic Secular Variation

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Earth Observation with CHAMP

Summary

New satellite data have led to increased resolution models of the geomagnetic secular variation (SV). Simple plots of the spectra of these models suggest an unphysical source depth above the core-mantle boundary (CMB). By taking a ratio of the main field and SV spectra, we argue that this result comes from the chosen spectral definition. The models are consistent with a CMB source for SV.

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References

  1. Bloxham J and Jackson A (1992) Time-dependent mapping of the magnetic field at the core-mantle boundary. J Geophys Res 97: 19,537–19,563.

    Google Scholar 

  2. Cain JC, Wang Z, Schmitz DR, and Meyer J (1989) The geomagnetic spectrum for 1980 and core-crustal separation. Geophys J 97: 443–447.

    Google Scholar 

  3. De Santis A, Barraclough DR, and Tozzi R. (2003) Spatial and temporal spectra of the geomagnetic field and their scaling properties. Phys Earth Planet Int 135:125–134.

    Article  Google Scholar 

  4. Holme R. and Bloxham J (1996) The treatment of attitude errors in satellite geomagnetic data. Phys Earth Planet Int 98: 221–233.

    Article  Google Scholar 

  5. Lowes FJ (1974) Spatial power spectrum of the main geomagnetic field, and extrapolation to the core. Geophys J R Astron Soc 36: 717–730.

    Google Scholar 

  6. McLeod MG (1985) Statistical theory of the geomagnetic field and its secular variation. EOS Trans. AGU 66(46): 878.

    Google Scholar 

  7. McLeod MG (1996) Spatial and temporal power spectra of the geomagnetic field. J Geophys Res 101: 2745–2763.

    Article  Google Scholar 

  8. Olsen N (2002) A model of the geomagnetic field and its secular variation for epoch 2000 estimated from Ørsted data. Geophys J Int 149: 454–462.

    Article  Google Scholar 

  9. Voorhies CV (2004) Narrow scale flow and a weak field by the top of Earth's core: evidence from Ørsted, Magsat and secular variation. J Geophys Res, in press.

    Google Scholar 

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© 2005 Springer-Verlag Berlin Heidelberg

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Holme, R., Olsen, N. (2005). The Spectrum of the Magnetic Secular Variation. In: Reigber, C., Lühr, H., Schwintzer, P., Wickert, J. (eds) Earth Observation with CHAMP. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-26800-6_52

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