Assimilation of the Observed SV with Geodynamo Modeling and Sensitivities of the Core Flow Beneath the Cmb
Abstract:
Determination of the observation operator for the velocity field is very complex, as the constraints from the observed SV are two orders of magnitude less than the velocity field state variables in dynamo simulation. Therefore, it depends on appropriate understanding of the responses of the core flow to the observed SV.
For this purpose, we carried out several assimilation experiments with and without assimilation of SV. In particular, the observed SV is only utilized for correcting the model forecasts in the magnetic field, leaving the velocity field forecast unconstrained. Our experiment shows that, the large-scale axisymmetric toroidal velocity responds the strongest to the observed SV, following by a suite of small-scale velocity components (with the span from spherical harmonic degree 10 to 20). The non-axisymmetric part of the poloidal flow is also very sensitive to the SV constraints. However, such responses are more evenly spread out from large to small-scale flow patterns. These assimilation results will be used for construction of the velocity field observational operator, and can be also applied to core-flow inversion studies in general.
