Identification of low-frequency fluctuations in the terrestrial magnetosheath

Journal Article · Fri Apr 01 04:00:00 EST 1994 · Journal of Geophysical Research

DOI:https://doi.org/10.1029/93JA03300· OSTI ID:121234

Song, P ^[1]; Russell, C T ^[2]; Gary, S P ^[3]

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1. National Center for Atmospheric Research, Boulder, CO (United States)
2. Univ. of California, Los Angeles, CA (United States)
3. Los Alamos National Lab., NM (United States)

On the basis of MHD theory the authors develop a scheme for distinguishing among the four low-frequency modes which may propagate in a high-{beta} anisotropic plasma such as the magnetosheath: the fast and slow magnetosonic, the Alfven, and mirror modes. The authors use four parameters: the ratio of transverse to compressional powers in the magnetic field, the ratio of the wave powers in the thermal pressure and in the magnetic field, the ratio of the perturbations in the thermal and magnetic pressures, and the ratio of the wave powers in the velocity and in the magnetic field. In the test case of an Active Magnetospheric Particle Tracer Explorers/Ion Release Module (AMPTE/IRM) magnetosheath pass near the Sun-Earth line downstream of a quasi-perpendicular shock, the four modes can be clearly distinguished both spatially and spectrally. Near the bow shock, the waves are Alfvenic in a large frequency range, 1 to 100 mHz. In the middle and inner magnetosheath, the waves below 10 mHz are Alfvenic. The fast mode waves occur in the higher-frequency end of the enhanced spectrum, 80 mHz for the middle magnetosheath and 55 mHz for the inner sheath. The wave enhancement in the intermediate frequencies is slow modes in the inner sheath and mirror modes in the middle sheath. This confirms the earlier report of the existence of the slow mode waves near the magnetopause. These slow waves provide evidence that the magnetopause is an active source of the waves in the sheath. The authors also show that the measured frequency of a wave is close to an invariant if the magnetosheath flow is in a steady state. Therefore changes in the frequencies of enhanced waves indicate emergence, or damping, or mode conversion of the waves. 50 refs., 5 figs., 1 tab.

• OSTI ID: 121234
• Journal Information: Journal of Geophysical Research, Journal Name: Journal of Geophysical Research Journal Issue: A4 Vol. 99; ISSN JGREA2; ISSN 0148-0227
• Country of Publication: United States
• Language: English

Related Subjects

66 PHYSICS
ALFVEN WAVES
FLUCTUATIONS
MAGNETOACOUSTIC WAVES
MAGNETOHYDRODYNAMICS
MAGNETOSHEATH
MILLI HZ RANGE