UPSTREAM ENERGETIC IONS AND ELECTRONS - BOW SHOCK-ASSOCIATED OR MAGNETOSPHERIC ORIGIN

被引：67

作者：

SCHOLER, M ^{[1
]}

HOVESTADT, D ^{[1
]}

IPAVICH, FM ^{[1
]}

GLOECKLER, G ^{[1
]}

机构：

[1] UNIV MARYLAND,DEPT PHYS & ASTRON,COLLEGE PK,MD 20742

来源：

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | 1981年 / 86卷 / NA11期

关键词：

D O I：

10.1029/JA086iA11p09040

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：9040 / 9046

页数：7

共 22 条

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[2]

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[5]

BIEBER JW, 1979, ESA SP148 EUR SPAC A, P131

[6] EVIDENCE FOR GREATER THAN 30-KEV ELECTRONS ACCELERATED IN SHOCK TRANSITION REGION BEYOND EARTHS MAGNETOSPHERIC BOUNDARY [J].

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[7] PROPERTIES OF ENERGETIC ELECTRONS OF MAGNETOSPHERIC ORIGIN IN THE MAGNETOSHEATH AND IN THE SOLAR WIND-CORRELATION WITH GEOMAGNETIC-ACTIVITY [J].

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[8] OBSERVATIONS OF 2 DISTINCT POPULATIONS OF BOW SHOCK IONS IN UPSTREAM SOLAR-WIND [J].

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[9]

GOSLING JT, 1979, C P AM I PHYS, V56, P81

[10] NUCLEAR AND IONIC CHARGE-DISTRIBUTION PARTICLE EXPERIMENTS ON ISEE-1 AND ISEE-C SPACECRAFT [J].

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FISK, LA ;

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KLECKER, B ;

OGALLAGHER, JJ ;

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ARBINGER, H ;

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IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, 1978, 16 (03) :166-175

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