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GEOPHYSICAL RESEARCH LETTERS,
VOL. 26, NO. 14,
PAGES 2151–2154,
1999
High Energy Ions and Electrons Upstream from the Earth’s Bow Shock and their Dependence on Geomagnetic Conditions: Statistical
Results Between Years 1982-1988
G. C. Anagnostopoulos
Demokritos University of Thrace, Department of Electrical and Computer Engineering, Xanthi 67100, Greece
G. Kaliabetsos
Demokritos University of Thrace, Department of Electrical and Computer Engineering, Xanthi 67100, Greece
G. Argyropoulos
Demokritos University of Thrace, Department of Electrical and Computer Engineering, Xanthi 67100, Greece
E. T. Sarris
Demokritos University of Thrace, Department of Electrical and Computer Engineering, Xanthi 67100, Greece
Abstract
We present initial results from a statistical analysis of 2034 energetic (50 -220 keV) ion events observed by the IMP-8 spacecraft
upstream from the Earth’s bow shock during a 6 years period. The most important findings are the following: (1) the percentage
Pe of high intensity energetic ion events accompanied by the presence of relativistic (≥ 220 keV) electrons is ∼80% (for all
geomagnetic conditions), and increases significantly with increasing the index Kp of geomagnetic activity, (2) high intensity energetic ion events most often (∼93%) show spectra extending up to energies
E>∼300 keV, (3) a percentage of ∼71.5% of events display non-inverse energy dispersion of ion intensities. The above results,
as well as additional results discussed in the text, suggest that a percentage as high as ∼80% of high intensity 50-220 keV
ion events in our statistical sample have an origin within the magnetosphere.
Received 18
November
1998;
accepted 23
March
1999.
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Citation: Anagnostopoulos, G. C., G. Kaliabetsos, G. Argyropoulos, and E. T. Sarris
(1999),
High Energy Ions and Electrons Upstream from the Earth’s Bow Shock and their Dependence on Geomagnetic Conditions: Statistical
Results Between Years 1982-1988,
Geophys. Res. Lett.,
26(14),
2151–2154.
Copyright 1999 by the American Geophysical Union.
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