BOUNDARY CONDITIONS ON MODEL SOLAR CHROMOSPHERES

被引：22

作者：

ATHAY, RG

机构：

[1] High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colo.

来源：

SOLAR PHYSICS | 1969年 / 9卷 / 01期

关键词：

D O I：

10.1007/BF00145727

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

It is shown that the gas pressure in the corona provides a rather stringent boundary condition on model chromospheres and limits the thickness of those regions of the chromosphere in which the temperature is less than 10 000 K to less than or about 2000 km. © 1969 D. Reidel Publishing Company.

引用

页码：51 / &

共 8 条

[1] ATHAY RG, 1967, ANN ASTROPHYS, V30, P669
[2] THEORETICAL LINE INTENSITIES .V. SOLAR UV EMISSION LINES OF HEAVY ELEMENTS
ATHAY, RG
[J]. ASTROPHYSICAL JOURNAL, 1966, 145 (03) : 784 - &
[3] ATHAY RG, IN PRESS
[4] ATHAY RG, 1955, ASTROPHYS J S, V1, P505
[5] Dupree A. K., 1967, SOL PHYS, V1, P229
[6] HENZE WJ, 1968, THESIS U COLORADO
[7] THERMODYNAMIC STRUCTURE OF THE OUTER SOLAR ATMOSPHERE .6. EFFECT OF DEPARTURES FROM THE SAHA EQUATION ON INFERRED PROPERTIES OF THE LOW CHROMOSPHERE
POTTASCH, SR
THOMAS, RN
[J]. ASTROPHYSICAL JOURNAL, 1960, 132 (01) : 195 - 201
[8] POTTASCH SR, 1967, B ASTRON I NETH, V19, P113

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