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：

SOLAR PHYSICS | 1976年 / 47卷 / 01期

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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[4]

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[5]

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[6] LINEAR STARK EFFECT DUE TO RESONANT INTERACTIONS OF STATIC AND DYNAMIC FIELDS [J].

COHN, A ;

BAKSHI, P ;

KALMAN, G .

PHYSICAL REVIEW LETTERS, 1972, 29 (06) :324-&

[7] BALMER-LINE ANOMALIES IN A TURBULENT-PLASMA [J].

GALLAGHER, CC ;

LEVINE, MA .

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 [J].

KUPERUS, M .

SOLAR PHYSICS, 1976, 47 (01) :79-90

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