EUV EMISSION, FILAMENT ACTIVATION AND MAGNETIC-FIELDS IN A SLOW-RISE FLARE

被引：69

作者：

RUST, DM

NAKAGAWA, Y

NEUPERT, WM

机构：

[1] SACRAMENTO PEAK OBSERV,SUNSPOT,NM

[2] NATL CTR ATMOSPH RES,HIGH ALTITUDE OBSERV,BOULDER,CO

[3] NASA,GODDARD SPACE FLIGHT CTR,LAB SOLAR PHYS,GREENBELT,MD

来源：

SOLAR PHYSICS | 1975年 / 41卷 / 02期

关键词：

D O I：

10.1007/BF00154077

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：397 / 414

页数：18

共 23 条

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[4]

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FRAZIER EN, 1972, SOL PHYS, V24, P98

[6] SOFT-X-RAY AND MICROWAVE OBSERVATIONS OF HOT REGIONS IN SOLAR-FLARES [J].

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[7]

Hyder C.L., 1967, SOPH, V2, P49

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

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[9] PRACTICAL REPRESENTATION OF MAGNETIC-FIELD [J].

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RAADU, MA .

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[10] SPATIAL-DISTRIBUTION OF SOFT-X-RAY AND EUV EMISSION ASSOCIATED WITH A CHROMOSPHERIC FLARE OF IMPORTANCE 1B ON AUGUST 2, 1972 [J].

NEUPERT, WM ;

THOMAS, RJ ;

CHAPMAN, RD .

SOLAR PHYSICS, 1974, 34 (02) :349-375

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