LINE FORMATION IN THE SOLAR CHROMOSPHERE .2. OPTICALLY THICK REGION OF THE CHROMOSPHERE-CORONA TRANSITION REGION OBSERVED WITH OSO-8

被引：11

作者：

LITES, BW

HANSEN, ER

SHINE, RA

机构：

[1] UNIV COLORADO,ATMOSPHER & SPACE PHYS LAB,BOULDER,CO 80309

[2] NASA,GODDARD SPACE FLIGHT CTR,GREENBELT,MD 20771

来源：

关键词：

D O I：

10.1086/157744

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：280 / 284

页数：5

共 8 条

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CHENG, CC ;

DOSCHEK, GA ;

FELDMAN, U .

[2] SOLAR C-III LINE INTENSITY RATIOS OBSERVED FROM SKYLAB [J].

COOK, JW ;

NICOLAS, KR .

[3]

FELDMAN U, 1978, ASTRON ASTROPHYS, V65, P215

[4] SEMI-EMPIRICAL MODEL OF THE UPPER FLARE CHROMOSPHERE [J].

LITES, BW ;

COOK, JW .

[5]

MAGEE NH, 1976, LA6691MS LOS AL REPT

[6]

ROTTMAN GJ, 1979, OSO8 LASP U COL FIN

[7] IONIZATION EQUILIBRIUM BALANCE [J].

VERNAZZA, JE ;

RAYMOND, JC .

[8]

WHITE OR, UNPUBLISHED