RELATIONSHIP BETWEEN HARD X-RAY AND EUV SOURCES IN SOLAR-FLARES

被引：35

作者：

KANE, SR

FROST, KJ

DONNELLY, RF

机构：

[1] NASA,GODDARD SPACE FLIGHT CTR,ASTRON & SOLAR PHYS LAB,GREENBELT,MD 20771

[2] NOAA,ENVIRONM RES LABS,SPACE ENVIRONM LAB,BOULDER,CO 80302

来源：

ASTROPHYSICAL JOURNAL | 1979年 / 234卷 / 02期

关键词：

D O I：

10.1086/157544

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：669 / 682

页数：14

共 31 条

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[2]

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

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[7] IMPULSIVE EXTREME-ULTRAVIOLET AND HARD X-RAY-EMISSION DURING SOLAR-FLARES [J].

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[8]

DONNELLY RF, 1970, ERL169SDL14 TR ESSA

[9] INTERRELATIONSHIP OF HARD X-RAY AND EUV BURSTS DURING SOLAR-FLARES [J].

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[10] EVIDENCE FROM HARD X-RAYS FOR 2-STAGE PARTICLE ACCELERATION IN A SOLAR FLARE [J].

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