FURTHER MEASUREMENTS OF EMISSION-LINE PROFILES IN SOLAR ULTRAVIOLET-SPECTRUM

被引：82

作者：

BOLAND, BC ^{[1
]}

DYER, EP ^{[1
]}

FIRTH, JG ^{[1
]}

GABRIEL, AH ^{[1
]}

JONES, BB ^{[1
]}

JORDAN, C ^{[1
]}

MCWHIRTER, RWP ^{[1
]}

MONK, P ^{[1
]}

TURNER, RF ^{[1
]}

机构：

[1] CULHAM LAB,ASTROPHYS RES DIV,APPLETON LAB,ABINGDON,OXFORDSHIRE,ENGLAND

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1975年 / 171卷 / 03期

关键词：

D O I：

10.1093/mnras/171.3.697

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：697 / &

共 34 条

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[2]

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[3]

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[5] HIGH RESOLUTION SOLAR ULTRAVIOLET SPECTRUM BETWEEN 200 AND 220 NM [J].

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[6]

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[7] NEW OBSERVATIONS OF SOLAR ULTRAVIOLET CHROMOSPHERE [J].

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PARKER, RW ;

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STEVENS, R .

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[8]

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[9] STRUCTURE OF CHROMOSPHERE-CORONA TRANSITION REGION FROM LIMB AND DISK INTENSITIES [J].

BURTON, WM ;

JORDAN, C ;

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WILSON, R .

PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY OF LONDON SERIES A-MATHEMATICAL AND PHYSICAL SCIENCES, 1971, 270 (1202) :81-&

[10]

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