H-ALPHA, HARD X-RAY, AND MICROWAVE EMISSIONS IN IMPULSIVE PHASE OF SOLAR-FLARES

被引：9

作者：

NEIDIG, DF

机构：

来源：

SOLAR PHYSICS | 1978年 / 57卷 / 02期

关键词：

D O I：

10.1007/BF00160111

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：385 / 398

页数：14

共 37 条

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CANFIELD, RC ;

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[3]

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[4] DEDUCTION OF ENERGY SPECTRA OF NON-THERMAL ELECTRONS IN FLARES FROM OBSERVED DYNAMIC SPECTRA OF HARD X-RAY BURSTS [J].

BROWN, JC .

SOLAR PHYSICS, 1971, 18 (03) :489-&

[5] THEORETICAL CHROMOSPHERIC FLARE SPECTRA .2. HYDROGEN EQUILIBRIUM FOR BROWNS (1973) MODELS FOR HEATING BY NONTHERMAL ELECTRONS [J].

CANFIELD, RC .

SOLAR PHYSICS, 1974, 34 (02) :339-348

[6] OSO-7 OBSERVATIONS OF SOLAR X-RAYS IN ENERGY-RANGE 10-100 KEV [J].

DATLOWE, DW ;

ELCAN, MJ ;

HUDSON, HS .

SOLAR PHYSICS, 1974, 39 (01) :155-174

[7]

DATLOWE DW, 1975, COMMUNICATION

[8] MAJOR HALPHA FLARES IN CENTERS OF ACTIVITY WITH VERY SMALL OR NO SPOTS [J].

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HEDEMAN, ER .

SOLAR PHYSICS, 1970, 13 (02) :401-&

[9]

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[10]

DONNELLY RF, 1973, S P HIGH ENERGY PHEN, P242

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