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MOESM16 of Unmodelled magnetic contributions in satellite-based models

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posted on 2016-06-28, 05:00 authored by Roberta Tozzi, Mioara Mandea, Paola De Michelis
Additional file 16: Figure B10. Structure of the dependence of Swarm B dZ residuals on IMF B y and B z according to the different IMF polarity sectors. Colour scale is given in arbitrary units (a.u.).

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    Earth, Planets and Space

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    Swarm magnetic vector dataInterplanetary Magnetic FieldMagnetic modelsField-aligned currentsPartial ring current

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