A GAS-DYNAMIC MODEL OF THE ROTATING SOLAR ATMOSPHERE

被引：1

作者：

NATH, O

机构：

[1] Department of Mathematics, S.C.P.G. College, Ballia, U.P.

来源：

SOLAR PHYSICS | 1991年 / 136卷 / 02期

关键词：

D O I：

10.1007/BF00146535

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A model is presented of a solar atmosphere which is heated by the periodic passage of shock waves. The outer atmosphere rotates and is assumed not to affect the strength of the shock waves. This constant shock strength hypothesis is used as the basis of the model of the outer solar atmosphere. From the model it is concluded that the chromospheric temperature rise and flow Mach number are slightly affected by the rotation of the atmosphere.

引用

页码：263 / 268

页数：6

共 15 条

[1]

BIERMANN L, 1948, Z ASTROPHYS, V25, P161

[2] SPECTROSCOPIC LIMITATION ON CORONAL HEATING MECHANISMS [J].