EMISSION-LINES IN WINGS OF CA II H AND K .1. INITIAL SOLAR OBSERVATIONS AND IMPLICATIONS

被引：8

作者：

CANFIELD, RC

STENCEL, RE

机构：

[1] SACRAMENTO PEAK OBSERV,SUNSPOT,NM

[2] UNIV MICHIGAN,DEPT ASTRON,ANN ARBOR,MI 48104

来源：

ASTROPHYSICAL JOURNAL | 1976年 / 209卷 / 02期

关键词：

D O I：

10.1086/154758

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：618 / 620

页数：3

共 24 条

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BROWN, DR ;

MANN, GR ;

MAUTER, HA .

SOLAR PHYSICS, 1972, 25 (01) :81-&

[2]

CANFIELD RC, 1971, ASTRON ASTROPHYS, V10, P64

[3] REVERSALS OF SELECTED CE 2 SOLAR LINES [J].

CANFIELD, RC .

ASTROPHYSICAL JOURNAL, 1969, 157 (1P1) :425-&

[4]

CANFIELD RC, 1971, ASTRON ASTROPHYS, V10, P54

[5]

CANFIELD RC, 1968, THESIS U COLORADO

[6]

DUNN RB, 1969, SKY TELESCOPE, V38, P368

[7]

DUNN RB, 1971, NBS353 SPEC PUBL, P71

[8] NEW IDENTIFICATIONS OF DISK EMISSION-LINES IN CA II H AND K-LINE WINGS [J].

ENGVOLD, O ;

HALVORSEN, HD .

SOLAR PHYSICS, 1973, 28 (01) :23-25

[9] POSSIBLE IDENTIFICATION OF NDII IN EMISSION IN ARCTURUS [J].

FOSBURY, RAE .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1971, 155 (02) :P7-&

[10]

GROSSIGALLEGOS H, 1971, SOL PHYS, V16, P120

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