K EMISSION-LINE WIDTHS AND SOLAR CHROMOSPHERE

被引：33

作者：

BAPPU, MK

SIVARAMAN, KR

机构：

来源：

SOLAR PHYSICS | 1971年 / 17卷 / 02期

关键词：

D O I：

10.1007/BF00150035

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：316 / +

页数：1

共 19 条

[1] LIFETIME OF SOLAR GRANULES [J].

BAHNG, J ;

SCHWARZSCHILD, M .

ASTROPHYSICAL JOURNAL, 1961, 134 (02) :312-&

[2]

BAPPU MKV, 1954, MATH STUDENT, V22, P43

[3]

DEJAGER C, 1959, HANDBUCH PHYSIK, V52

[4] DETAILED STUDY OF THE DEVELOPMENT OF AN ACTIVE SOLAR REGION, 1954 AUGUST 20-27 [J].

DODSON, HW ;

HEDEMAN, ER .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1956, 116 (04) :428-&

[5] OBSERVATIONAL STUDY OF MACROSCOPIC INHOMOGENEITIES IN SOLAR ATMOSPHERE .4. VELOCITY AND INTENSITY FLUCTUATIONS OBSERVED IN K LINE [J].

JENSEN, E ;

ORRALL, FQ .

ASTROPHYSICAL JOURNAL, 1963, 138 (01) :252-&

[6]

KURIYAN PP, 1967, 172 KOD OBS B

[7] OBSERVATIONS OF SOLAR MAGNETIC FIELDS IN PLAGE REGIONS [J].

LEIGHTON, RB .

ASTROPHYSICAL JOURNAL, 1959, 130 (02) :366-&

[8]

LILLER, 1968, ASTROPHYS J, V151, P589

[9] SOLAR H-LINES K-LINES [J].

LINSKY, JL ;

AVRETT, EH .

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1970, 82 (485) :169-+

[10]

PASACHOFF JM, 1970, SOL PHYS, V12, P203

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