WHISTLER-MODE CHORUS AND MORNINGSIDE AURORAE

被引：49

作者：

INAN, US ^{[1
]}

CHIU, YT ^{[1
]}

DAVIDSON, GT ^{[1
]}

机构：

[1] LOCKHEED PALO ALTO RES LABS,SPACE SCI LAB,PALO ALTO,CA 94304

来源：

GEOPHYSICAL RESEARCH LETTERS | 1992年 / 19卷 / 07期

关键词：

D O I：

10.1029/92GL00402

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

摘要：

Quasi-electrostatic ELF/VLF chorus emissions immediately above the equatorial half-gyrofrequency, observed to propagate with wave normal angle (psi) within 0.4-1.2-degrees of the resonance cone (psi(r) [Muto et al., 1987], are shown to efficiently resonate with 0.1-10 keV electrons. These waves may thus be important in driving the relatively low energy (< 10 keV) component of pulsating aurorae and the morning-side diffuse aurorae (approximately 1 keV).

引用

页码：653 / 656

页数：4

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