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GEOPHYSICAL RESEARCH LETTERS,
VOL. 29, NO. 5,
1058,
doi:10.1029/2001GL013988,
2002
Solar cycle and geomagnetic N+1/O+1 variation in outer dayside magnetosphere: Possible relation to topside ionosphere
S. P. Christon
Focused Analysis and Research,
Columbia,
Maryland,
USA
U. Mall
Max Planck-Institute fur Aeronomie,
Katlenburg-Lindau,
Germany
T. E. Eastman
Plasmas International,
Silver Spring,
Maryland,
USA
G. Gloeckler
Department of Physics,
University of Maryland,
College Park,
USA
A. T. Y. Lui
JHU/APL,
Laurel,
Maryland,
USA
R. W. McEntire
JHU/APL,
Laurel,
Maryland,
USA
E. C. Roelof
JHU/APL,
Laurel,
Maryland,
USA
Abstract
O+1 and N+1 are important ring current ions in great magnetic storms. We study ∼10–210 keV/e O+1 and N+1 in dayside outer ring current (ORC) at ∼9–15 RE using Geotail's EPIC/STICS ion spectrometer. We find: average N+1/O+1 (ΓN/O) varies by ∼2 over a solar cycle, ∼40% (∼20%) at solar minimum (maximum); individual ΓN/O values range from ∼0.15 (moderate solar maximum storm) to ∼1 (18-hr solar minimum superquiet interval); and N+1 is third in importance after H+ and O+1 during two moderate storms (Dstmin ∼ −80 nT, ∼25% great storm intensity), one at minimum, one maximum. High-latitude topside ionospheric AE-D/MIMS ion composition
data form a baseline reference used to argue that ORC ΓN/O variations generally reflect and may be partially explained by topside ionospheric density ΓN/O spatial variations.
Published 8
March
2002.
Index Terms: 2736 Magnetospheric Physics: Magnetosphere/ionosphere interactions; 2730 Magnetospheric Physics: Magnetosphere—inner; 2778 Magnetospheric Physics: Ring current; 2788 Magnetospheric Physics: Storms and substorms.
Read Full Article (file size: 174420 bytes) Cited by
Citation: Christon, S. P., U. Mall, T. E. Eastman, G. Gloeckler, A. T. Y. Lui, R. W. McEntire, and E. C. Roelof
(2002),
Solar cycle and geomagnetic N+1/O+1 variation in outer dayside magnetosphere: Possible relation to topside ionosphere,
Geophys. Res. Lett.,
29(5),
1058,
doi:10.1029/2001GL013988.
Copyright 2002 by the American Geophysical Union.
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