EGU22-7541
https://doi.org/10.5194/egusphere-egu22-7541
EGU General Assembly 2022
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.

The detection of the magnetic fields induced by ocean circulation - An observing system simulation experiment

Aaron Hornschild1, Jan Saynisch-Wagner1, Julien Baerenzung2, Christopher Irrgang1, and Maik Thomas1,3
Aaron Hornschild et al.
  • 1GFZ German Research Centre for Geosciences, Section 1.3: Earth System Modelling, Potsdam, Germany
  • 2Universität Potsdam, Institute for Mathematics, Potsdam, Germany
  • 3Freie Universität Berlin, Institute of Meteorology, Berlin, Germany

The movement of conductive seawater through Earth's magnetic field leads to electromagnetic induction processes in the oceans. The resulting radial magnetic fields have been successfully modeled and, in the case of tidal-induced magnetic fields, also identified in satellite magnetometer data. However, the magnetic signals caused by ocean circulation have still remained unobserved.
We introduce a new method to detect these signals using an observing system simulation experiment. Our approach relies on a Kalman filter-based assimilation of satellite magnetometer data. A key aspect of identifying ocean-induced signals is separating them from other magnetic contributions. For this separation, we used both estimations of the temporal behavior and spatial constraints as prior information. The observing system simulation experiment allows us to evaluate the proposed method.  
We present the results of this evaluation and report on the detectability of magnetic fields induced by ocean circulation.

How to cite: Hornschild, A., Saynisch-Wagner, J., Baerenzung, J., Irrgang, C., and Thomas, M.: The detection of the magnetic fields induced by ocean circulation - An observing system simulation experiment, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-7541, https://doi.org/10.5194/egusphere-egu22-7541, 2022.

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