DOPPLER WAVELENGTH SHIFTS OF ULTRAVIOLET SPECTRAL-LINES IN SOLAR ACTIVE REGIONS

被引：55

作者：

FELDMAN, U ^{[1
]}

COHEN, L ^{[1
]}

DOSCHEK, GA ^{[1
]}

机构：

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

来源：

ASTROPHYSICAL JOURNAL | 1982年 / 255卷 / 01期

关键词：

D O I：

10.1086/159833

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：325 / 328

页数：4

共 12 条

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[2]

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[3]

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[4]

DERE KP, 1982, SOLAR PHYS

[5]

DERE KP, 1982, MONOGRAPH NASA SKYLA, pCH6

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[8] THE USE OF SPECTRAL EMISSION-LINES IN THE DIAGNOSTICS OF HOT SOLAR PLASMAS [J].

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[9] SEARCH FOR A TURBULENT-FREE REGION IN SOLAR TRANSITION ZONE [J].

FELDMAN, U ;

DOSCHEK, GA .

ASTROPHYSICAL JOURNAL, 1977, 216 (03) :L119-L121

[10] PRELIMINARY-RESULTS FROM ORBITING SOLAR OBSERVATORY 8 - PERSISTENT VELOCITY-FIELDS IN CHROMOSPHERE AND TRANSITION REGION [J].

LITES, BW ;

BRUNER, EC ;

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