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Geomagnetic Virtual Observatories

 

Figure 1: The cylindrical region around a Geomagnetic Virtual Observatory (GVO) where satellite data are collected. Image: DTU Space Figure 2: Comparison of a secular variation data from a virtual observatory (VO, red dots) over Hermanus, South Africa with the data from the Hermanus geomagnetic observatory (GO, black dots) from the CHAMP and Swarm satellites. The agreement is excellent. Image:  DTU Space

In collaboration with Danish Technical University (DTU Space), BGS have won a contract from the European Space Agency to produce a new Swarm product called Geomagnetic Virtual Observatories (GVO).

Unlike ground observatories, which are stationary, the three Swarm magnetic satellites move at around 8 km/second and only revisits the same location on the surface once every 4 months. This makes it difficult to directly compare satellite and ground observatory data. To overcome this, we intend to create a set of 'virtual observatories' in space.

These are created in three steps. First, we collect all the satellite data that pass within 700 km of an defined point in space (at 400 km) [Figure 1]. We do this for 300 points on an equal area grid across the globe. Secondly, we subtract off the core field and find the robust 'average' of the residuals. Finally, we add back on the core field to get the magnetic field vector at each virtual observatory.

If we place a GVO over a ground observatory, the comparison between the rate of change of the magnetic field (so-called secular variation) is excellent. Figure 2 shows an example for the Hermanus observatory in South Africa.

However, GVO data are not perfect and often contain contamination from the ionosphere and magnetosphere, so there are further processing steps to extract the purely core field signal.

The final product for ESA will consist of several GVO grids with various levels of processing and cleaning applied to them. These will be useful for researchers studying the dynamics of the outer core (e.g. fluid flow or secular acceleration).

The project kicked off on 3rd June 2019 and will run until June 2020.

Contact

For more information please contact Dr Ciaran Beggan.

References/Further reading

  • Beggan, C. D., K. A. Whaler and S. Macmillan (2009), Biased residuals of core flow models from satellite-derived 'virtual observatories', Geophysical Journal International, Volume 177 (2), 463-475, doi:10.1111/j.1365-246X.2009.04111.x
  • Barrois, O., M. D. Hammer, C. C. Finlay, Y. Martin and N. Gillet, (2018) Assimilation of ground and satellite magnetic measurements: inference of core surface magnetic and velocity field changes, Geophysical Journal International, 215 (1), 695-712, doi:10.1093/gji/ggy297
  • Cox, G. A., Brown, W. J., Billingham, L., & Holme, R. (2018), MagPySV: A Python package for processing and denoising geomagnetic observatory data. Geochemistry, Geophysics, Geosystems, 19, 3347-3363. doi:10.1029/2018GC007714
  • Mandea, M., and Olsen, N. (2006), A new approach to directly determine the secular variation from magnetic satellite observations, Geophys. Res. Lett., 33, L15306, doi:10.1029/2006GL026616.