A PRELIMINARY INTERPRETATION OF STELLAR CHROMOSPHERIC CA II EMISSION VARIATIONS WITHIN THE FRAMEWORK OF STELLAR DYNAMO THEORY

被引:90
作者
DURNEY, BR
MIHALAS, D
ROBINSON, RD
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D O I
10.1086/130878
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P1 [天文学];
学科分类号
0704 ;
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页码:537 / 543
页数:7
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共 24 条
[1]  
BELVEDERE G, 1980, ASTRON ASTROPHYS, V91, P328
[2]  
DURNEY BR, 1981, AP J
[3]   MULTI-CHANNEL MAGNETOGRAPH OBSERVATIONS .3. FACULAE [J].
FRAZIER, EN .
SOLAR PHYSICS, 1971, 21 (01) :42-&
[5]  
KRAUSE F, 1976, BASIC MECHANISMS SOL, P305
[6]   SOLAR H-LINES K-LINES [J].
LINSKY, JL ;
AVRETT, EH .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1970, 82 (485) :169-+
[7]   STELLAR MODEL CHROMOSPHERES .10. HIGH-RESOLUTION, ABSOLUTE FLUX PROFILES OF THE CA-II H-LINE AND K-LINE IN STARS OF SPECTRAL TYPES-F0-M2 [J].
LINSKY, JL ;
WORDEN, SP ;
MCCLINTOCK, W ;
ROBERTSON, RM .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1979, 41 (01) :47-74
[8]  
Moffatt H.K., 1978, MAGNETIC FIELD GENER
[9]  
Parker E.N., 1979, COSMICAL MAGNETIC FI
[10]   GENERATION OF MAGNETIC-FIELDS IN ASTROPHYSICAL BODIES .10. MAGNETIC BUOYANCY AND SOLAR DYNAMO [J].
PARKER, EN .
ASTROPHYSICAL JOURNAL, 1975, 198 (01) :205-209