Irregular, long-period boundary oscillations beyond approximately 100 R(sub e): GEOTAIL plasma observations

Details Irregular, long-period boundary oscillations beyond approximately 100 R(sub e): GEOTAIL plasma observations Irregular, long-period boundary oscillations beyond approximately 100 R(sub e): GEOTAIL plasma observations

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994georl..21.2979s&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 21, no. 25, p. 2979-2982

Physics

2

Flow Velocity, Geomagnetic Tail, Magnetohydrodynamic Flow, Periodic Variations, Plasma Density, Plasma Oscillations, Satellite Observation, Space Plasmas, Azimuth, Density Distribution, Geophysical Satellites, Velocity Distribution

Scientific paper

Near the tail boundary beyond about 100 Re, GEOTAIL often measures irregular, long-period oscillations in plasma velocity and density. Flow speed and density oscillate between magnetosheath values and values an order of magnitude less. The oscillations can persist for days. A typical oscillation lasts 100 minutes, but the range is large. The oscillations are highly asymmetric in that the increasing phase of the oscillation is an order of magnitude faster than the decreasing phase. This asymmetry shows that they are a distinct class of oscillations, not previously explicitly reported, and that they are not mere consequences of tail flapping in a variable solar wind. The changes in flow direction through an oscillation imply that the oscillation results from a motion of the boundary toward and away from the spacecraft with an amplitude between 5 and 10 R(sub e). A consideration of options suggests that the most plausible cause of these oscillations is the 'breathing' of the magnetotail that attends the substorm cycle.

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