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

页码：3167 / 3168

页数：2

共 4 条

[1] Cuperman S., 1970, Cosmic Electrodynamics, V1, P205
[2] HEAT-CONDUCTION IN A TURBULENT MAGNETIC-FIELD, WITH APPLICATION TO SOLAR-WIND ELECTRONS
HOLLWEG, JV
JOKIPII, JR
[J]. JOURNAL OF GEOPHYSICAL RESEARCH, 1972, 77 (19): : 3311 - +
[3] SOLAR WIND PROTON PROPERTIES - VELA-3 OBSERVATIONS FROM JULY 1965 TO JUNE 1967
HUNDHAUSEN, AJ
BAME, SJ
ASBRIDGE, JR
SYDORIAK, SJ
[J]. JOURNAL OF GEOPHYSICAL RESEARCH, 1970, 75 (25): : 4643 - +
[4] MONTGOMERY MD, 1971, SOLAR WIND C U CALIF