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NASA NTRS · 20010021221

Magnetosheath Flow Anomalies in 3-D

Abstract

Measurements of the plasma and magnetic field with high temporal resolution on the Interball Tail probe reveal many flow anomalies in the magnetosheath. They are usually seen as flow direction and number density variations, accompanied by magnetic field discontinuities. Large flow anomalies with number density variations of factor of 2 or more and velocity variations of 100 km/s or more are seen with periodicity of about I per hour. The cases of flow anomalies following in succession are also observed, and suggest their decay while propagating through the magnetosheath. Some magnetospheric disturbances observed in the outer magnetosphere after the satellite has crossed the magnetopause on the inbound orbit suggest their association with magnetosheath flow anomalies observed in the magnetosheath prior to magnetopause crossing.

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BibTeXRIS

Vaisberg, O. L., Burch, J. L., Smirnov, V. N., Avanov, L. A., Moore, T. E., Waite, J. H., Jr., Skalsky, A. A., Borodkova, N. L., Coffey, V. N., Gallagher, D. L., Rose, M. Franklin. 2000-01-01. Magnetosheath Flow Anomalies in 3-D. https://ntrs.nasa.gov/citations/20010021221

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