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Fig. 2. | Earth, Planets and Space

Fig. 2.

From: Solar cycle dependence of quiet-time magnetospheric currents and a model of their near-Earth magnetic fields

Fig. 2.

Breakdown of the parts contributing to the uniform field in SM coordinates. The observed annual mean values of SM fields are presented as plus signs. The model estimate of the −ZSM component is drawn as thick curve. This is composed of a constant bias (dashed-dotted), an Est dependent component (thin line), and a solar cycle dependent component approximated by the F10.7 index delayed by 20 months (dashed).

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