POSSIBLE SPECTRAL DIAGNOSTICS FOR TURBULENT ELECTRIC-FIELDS IN SOLAR-FLARES

被引：19

作者：

BAKSHI, P ^{[1
]}

KALMAN, G ^{[1
]}

机构：

[1] BOSTON COLL,DEPT PHYS,CHESTNUT HILL,MA 02167

来源：

关键词：

D O I：

10.1007/BF00152268

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：307 / 316

页数：10

共 14 条

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[2] BAKSHI P, 1974, B AM PHYS SOC, V19, P975
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[5] Blokhintsev D, 1933, PHYS SOW UNION, V4, P501
[6] LINEAR STARK EFFECT DUE TO RESONANT INTERACTIONS OF STATIC AND DYNAMIC FIELDS
COHN, A
BAKSHI, P
KALMAN, G
[J]. PHYSICAL REVIEW LETTERS, 1972, 29 (06) : 324 - &
[7] BALMER-LINE ANOMALIES IN A TURBULENT-PLASMA
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LEVINE, MA
[J]. PHYSICAL REVIEW LETTERS, 1973, 30 (19) : 897 - 900
[8] HOGABOOM R, 1975, THESIS BOSTON COLLEG
[9] KAPLAN SA, 1973, PLASMA ASTROPHYSICS, P122
[10] ROLE OF PLASMA TURBULENCE IN DEVELOPMENT OF SOLAR-FLARES
KUPERUS, M
[J]. SOLAR PHYSICS, 1976, 47 (01) : 79 - 90