On the absence of plasma wave emissions and the magnetic field orientation in the distant magnetosheath
Article first published online: 7 DEC 2012
Copyright 1994 by the American Geophysical Union.
Geophysical Research Letters
Volume 21, Issue 24, pages 2761–2764, 1 December 1994
How to Cite
- Issue published online: 7 DEC 2012
- Article first published online: 7 DEC 2012
- Manuscript Accepted: 8 JUN 1994
- Manuscript Received: 2 MAR 1994
In early September, 1983 ISEE-3 made a long traversal of the distant dawnside magnetosheath starting near x = −150 RE downstream. The distant magnetosheath often contains moderately intense plasma wave emissions at frequencies from several hundred Hz to 5 kHz. However, over time scales of many days, a clear correlation exists between the occurrence of the plasma waves and the cone angle (θxB) between the magnetic field and the plasma flow velocity (x-direction). For θxB large (small), the plasma wave amplitudes are near background (high). Sudden ( < 1 minute) changes in the local magnetic field orientation produce correspondingly sudden changes in the wave amplitudes. Statistically, the wave amplitudes decrease continuously with increasing θxB.