The motion and magnetic structure of the plasma sheet near 30RE

Details The motion and magnetic structure of the plasma sheet near 30RE The motion and magnetic structure of the plasma sheet near 30RE

May 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974p%26ss...22..673b&link_type=abstract

Planetary and Space Science, Volume 22, Issue 5, p. 673-686.

Computer Science

7

Scientific paper

Data taken by the NASA-GSFC magentometer aboard the Explorer 34 satellite are analysed in an effort ascertain the average motion and magnetic field structure of the plasma sheet near 30RE. We find that the flapping motion of the plasma sheet in the solar ecliptic Z-coordinate is characterized by a typical speed of 90 km/sec and an amplitude of +/-2RE. Results suggest that there exists a layer of nearly uniform cross-tail current density in the central region of the plasma sheet approx 2. 3-2. 6RE thick within which the solar-magnetospheric X-component of the magnetic field changes from 10γ to - 10γ. Near the centre of the plasma sheet, the average value of the Z-component of the field is 2γ. The analysis does not suggest a strong dependence of the magnetic-field configuration on Kp.

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