ROLE OF FLUCTUATIONS IN INTERPLANETARY MAGNETIC-FIELD ON HEAT-CONDUCTION IN SOLAR-WIND

被引：4
作者：
CUPERMAN, S
METZLER, N
机构：
[1] NOAA,ENVIRONM RES LABS,SPACE ENVIRONM LAB,BOULDER,CO 80302
[2] TEL AVIV UNIV,DEPT PHYS & ASTRON,RAMAT AVIV,ISRAEL
[3] UNIV COLORADO,COOPERAT INST RES ENVIRONM SCI,BOULDER,CO 80302
来源：
JOURNAL OF GEOPHYSICAL RESEARCH | 1973年 / 78卷 / 16期
关键词：
D O I：
10.1029/JA078i016p03167
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：
引用
收藏
页码：3167 / 3168
页数：2
相关论文
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Cuperman S., 1970, Cosmic Electrodynamics, V1, P205
[2]   HEAT-CONDUCTION IN A TURBULENT MAGNETIC-FIELD, WITH APPLICATION TO SOLAR-WIND ELECTRONS [J].
HOLLWEG, JV ;
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[3]   SOLAR WIND PROTON PROPERTIES - VELA-3 OBSERVATIONS FROM JULY 1965 TO JUNE 1967 [J].
HUNDHAUSEN, AJ ;
BAME, SJ ;
ASBRIDGE, JR ;
SYDORIAK, SJ .
JOURNAL OF GEOPHYSICAL RESEARCH, 1970, 75 (25) :4643-+
[4]  
MONTGOMERY MD, 1971, SOLAR WIND C U CALIF
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