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P. Schmoldt, PhD - MTNet - DIAS

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2.2. Electric currents in the magnetosphere<br />

Fig. 2.8.: Projection of the dip equator (dashed) and the geomagnetic equator (dip-pointed) onto the Earth’s surface; from Mareschal<br />

[1986].<br />

Fig. 2.9.: Equivalent current system for lunar daily variations L exhibiting two separate current loops on the day-lit side of either<br />

hemisphere (U.T.: Universal time); from Malin [1973]<br />

three degrees around the dip equator [e.g. Vozoff , 1987; Padilha et al., 1997; Padilha,<br />

1999; Brasse, 2003], i.e. the region of horizontal geomagnetic field lines that are usually<br />

in close proximity to the Earth’s equator (Fig. 2.8). Amplitudes of regular solar daily<br />

variations can be enhanced through such irregular variations by up to 20 nT on disturbed<br />

days S D [Schmucker, 1985], having serious effects on local MT observations [e.g. Hesse,<br />

1982; Padilha et al., 1997; Padilha, 1999].<br />

Lunar daily variation<br />

Lunar daily variations are due to tidal effects in the oceans and atmosphere of the Earth<br />

originating from the Moon orbiting the Earth, thereby forcing tidal currents to move<br />

across field lines inducing effects on the magnetosphere. Such effects can be represented<br />

by an equivalent current system exhibiting two characteristic separate current loops on the<br />

day-lit side of either hemisphere [Schmucker, 1985] (Fig. 2.9). The effect of lunar daily<br />

variations is commonly neglected given its minor amplitude in comparison with S q and<br />

the effect of thermal instabilities in the recording of the MT electric components which<br />

both occur in a similar frequency range.<br />

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