DOES H- TRULY COOL THE SOLAR CHROMOSPHERE

被引：10

作者：

AYRES, TR ^{[1
]}

机构：

[1] NBS,BOULDER,CO 80309

来源：

SOLAR PHYSICS | 1980年 / 68卷 / 01期

关键词：

D O I：

10.1007/BF00153271

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：125 / 133

页数：9

共 20 条

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[2]

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REINHARDT, WP .

PHYSICAL REVIEW A, 1976, 14 (06) :2159-2173

[4]

CAYREL R, 1963, CR HEBD ACAD SCI, V257, P3309

[5] IONIZATION EQUILIBRIUM AND RADIATIVE COOLING OF A LOW-DENSITY PLASMA [J].

COX, DP ;

TUCKER, WH .

ASTROPHYSICAL JOURNAL, 1969, 157 (3P1) :1157-&

[6] ON DEPENDENCE OF TE UPON QUANTITY VERSUS QUALITY OF RADIATION FIELD IN A STELLAR ATMOSPHERE [J].

GEBBIE, KB ;

THOMAS, RN .

ASTROPHYSICAL JOURNAL, 1970, 161 (01) :229-+

[7] ACOUSTIC DISSIPATION AND H- RADIATION IN THE SOLAR CHROMOSPHERE .2. [J].

KALKOFEN, W ;

ULMSCHNEIDER, P .

ASTROPHYSICAL JOURNAL, 1979, 227 (02) :655-663

[8] PRELIMINARY THEORETICAL LINE-BLANKETED MODEL SOLAR PHOTOSPHERE [J].

KURUCZ, RL .

SOLAR PHYSICS, 1974, 34 (01) :17-23

[9] DISSOCIATION EQUILIBRIUM OF H- IN STELLAR ATMOSPHERES [J].

LAMBERT, DL ;

PAGEL, BEJ .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1968, 141 (03) :299-&

[10]

LINSKY JL, 1979, STELLAR TURBULENCE, V51, P248

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