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The factors ε n m are the SHE coefficients describing the frequency content of the inducing source.
We consider a large-scale magnetospheric source, which we parametrize with 15 low-degree SHE coefficients ε n m (n≤3, |m|≤3).
The CI aims to separate magnetic contributions from various sources (originating in the core, lithosphere, ionosphere and magnetosphere) in the form of corresponding SHE coefficients.
Time series of internal SHE coefficients are synthesized by simulating induction in the target conductivity model (Subsection 3.1), cf. companion paper by Puthe and Kuvshinov (2013).
The external and internal SHE coefficients of the magnetic potential due to magnetospheric sources recovered by the CI constitute a realistic test data set for our inversion scheme.
The data consist of internal SHE coefficients up to degree and order 5 at periods between two days and two months.
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