Including the Temporal Dimension in the SECS Technique
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2020-06-08Resumen
The equivalent source method of Spherical Elementary Current Systems (SECS) has
contributed valuable results for spatial magnetic interpolation purposes where no observations are
available, as well as for modeling equivalent currents both in the ionosphere and in the subsurface, thus
providing a separation between external and internal sources. It has been successfully applied to numerous
Space Weather (SW) events, whereas some advantages have been reported over other techniques such as
Fourier or Spherical (Cap) Harmonic Analysis. Although different modalities of SECS exist (either 1‐D, 2‐D,
or 3‐D) depending on the number of space dimensions involved, the method provides a sequence of
instantaneous pictures of the source current. We present an extension of SECS consisting in the introduction
of a temporal dependence in the formulation based on a cubic B‐splines expansion. The technique thus adds
one dimension, becoming 4‐D in general (e.g., 3‐D + t), and its application is envisaged for, though not
restricted to, the analysis of past events including heterogeneous geomagnetic data sets, such as those
containing gaps, different sampling rates or diverse data sources. A synthetic model based on the SW
Modeling Framework is used to show the efficacy of the extended scheme. We apply this method to
characterize the current systems of past and significant SW events producing geomagnetically induced
currents, which we exemplify with an outstanding geomagnetic sudden commencement occurred on 24
March 1991.
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Space Weather, 18, e2020SW002491
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