Cusp energetic particle events measured by POLAR spacecraft

被引:27
|
作者
Fritz, TA
Chen, JS
Sheldon, RB
Spence, HE
Fennell, JF
Livi, S
Russell, CT
Pickett, JS
机构
[1] Boston Univ, Ctr Space Phys, Boston, MA 02215 USA
[2] Aerosp Corp, Los Angeles, CA 90009 USA
[3] Max Planck Inst Aeron, D-37189 Katlenburg Lindau, Germany
[4] Univ Calif Los Angeles, Inst Geophys & Planetary Phys, Los Angeles, CA 90095 USA
[5] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
来源
PHYSICS AND CHEMISTRY OF THE EARTH PART C-SOLAR-TERRESTIAL AND PLANETARY SCIENCE | 1999年 / 24卷 / 1-3期
基金
美国国家航空航天局;
关键词
D O I
10.1016/S1464-1917(98)00020-8
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The Charge and Mass Magnetospheric Ion Composition Experiment (CAMMICE) on board the POLAR spacecraft observed more than 70 cusp energetic particle (CEP) events in 1996. All of these events were associated with a decrease in the magnitude of the local magnetic field measured by the Magnetic Field Experiment (MFE) on POLAR. This is an important discovery, which reveals six interesting features for the CEP events: (1) They all were detected in the dayside at high latitude near apogee; (2) their energies were in excess of 2.4 MeV; (3) an individual. CEP event could last for hours; (4) the event-averaged intensity of 1-200 keV/e helium was anticorrelated with the magnitude of the local geomagnetic field but correlated with the turbulent magnetic energy density; (5) the events were associated with an enhancement of the low frequency electromagnetic noise; and (6) a possible seasonal variation was found for the occurrence rate of the events with a maximum in September. The measured high charge state of helium and oxygen ions in the CEP events indicates a solar source for these particles. A possible explanation is that the energetic helium ions are energized from lower energy helium by a local acceleration mechanism associated within the high-altitude dayside cusp. These observations represent a discovery of a major acceleration region of the magnetosphere. (C) 1998 Elsevier Science Ltd. All rights reserved.
引用
收藏
页码:135 / 140
页数:6
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