DYNAMICAL MODEL OF CORONA

被引：6

作者：

BROWNE, SL ^{[1
]}

BESSEY, RJ ^{[1
]}

机构：

[1] UNIV WYOMING,DEPT PHYS & ASTRONOM,LARAMIE,WY 82070

来源：

SOLAR PHYSICS | 1973年 / 31卷 / 02期

关键词：

D O I：

10.1007/BF00152813

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：351 / 375

页数：25

共 17 条

[1]

BURTON WM, 1969, P C NATIONAL CTR ATM

[2] RADIO MODEL OF TRANSITION LAYER IN SOLAR ACTIVE REGIONS [J].

CHIUDERI, C ;

CHIUDERI.F ;

NOCI, G .

SOLAR PHYSICS, 1971, 17 (02) :369-&

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

COX, DP ;

TUCKER, WH .

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

[4]

Fox L, 1962, NUMERICAL SOLUTION O

[5] HARVARD-SMITHSONIAN REFERENCE ATMOSPHERE [J].

GINGERICH, O ;

NOYES, RW ;

KALKOFEN, W ;

CUNY, Y .

SOLAR PHYSICS, 1971, 18 (03) :347-+

[6]

JORDAN C, 1965, THESIS U LONDON

[7]

KUPERUS M, 1969, SPACE SCI REV, V9, P713, DOI 10.1007/BF00174033

[8] OBSERVED PROPERTIES OF INTERPLANETARY PLASMA [J].

NESS, NF .

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1968, 6 :79-&

[9] STRUCTURE OF SOLAR CORONA [J].

NEWKIRK, G .

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1967, 5 :213-&

[10]

OSTER L, 1956, Z ASTROPHYS, V40, P28

← 1 2 →