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JOURNAL OF GEOPHYSICAL RESEARCH,
VOL. 107, NO. A8,
1206,
doi:10.1029/2001JA000284,
2002
Observations of bow shock and magnetopause crossings from geosynchronous orbit on 31 March 2001
Daniel M. Ober
Mission Research Corporation,
Nashua,
New Hampshire,
USA
M. F. Thomsen
Los Alamos National Laboratory,
Los Alamos,
New Mexico,
USA
N. C. Maynard
Mission Research Corporation,
Nashua,
New Hampshire,
USA
Abstract
On 31 March 2001, significant enhancements in both the strength of the interplanetary magnetic field and the solar wind dynamic
pressure pushed the magnetopause and bow shock inside of geosynchronous orbit. We present here observations of the unshocked
solar wind observed with the Los Alamos magnetospheric plasma analyzer on geosynchronous satellite 1994-084 near local noon.
The magnetosheath was observed intermittently at geosynchronous satellites 1991-080, 1994-084, and LANL-01A, across much of
the dayside magnetosphere. Comparisons with theory of the observed bow shock and magnetopause locations at geosynchronous
orbit near noon are in reasonable agreement. Using nearly simultaneous observations of the magnetopause and bow shock locations
at 0451 UT, we have tested models for the thickness of the magnetosheath and flaring of the magnetopause at that time. Using
the least flared of the magnetopause models, the estimated thickness of the magnetosheath would be thicker than would be predicted
by either the gas dynamic solution of
Spreiter et al. [1966]
or the MHD simulations of
Cairns and Lyon [1996]
. Alternatively, placing the location of the magnetopause at the nose of the magnetosphere in conformance with the thickness
of the magnetosheath from
Cairns and Lyon [1996]
requires less flaring on the flanks of the magnetosphere than currently present in the empirical models. The models also
have difficulty predicting the other observed magnetopause crossings far from local noon apparently due to excessive flaring
of the models for the conditions on this day.
Published 27
August
2002.
Index Terms: 2740 Magnetospheric Physics: Magnetospheric configuration and dynamics; 2784 Magnetospheric Physics: Solar wind/magnetosphere interactions; 2724 Magnetospheric Physics: Magnetopause, cusp, and boundary layers; 2728 Magnetospheric Physics: Magnetosheath.
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Citation: Ober, D. M., M. F. Thomsen, and N. C. Maynard
(2002),
Observations of bow shock and magnetopause crossings from geosynchronous orbit on 31 March 2001,
J. Geophys. Res.,
107(A8),
1206,
doi:10.1029/2001JA000284.
Copyright 2002 by the American Geophysical Union.
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