ON DIFFERENTIAL ROTATION WITH HEIGHT IN SOLAR ATMOSPHERE

被引：36

作者：

LIVINGST.WC

机构：

[1] Kitt Peak National Observatory, Tucson, Ariz.

来源：

SOLAR PHYSICS | 1969年 / 9卷 / 02期

关键词：

D O I：

10.1007/BF02391670

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Spectroscopic measurements of solar rotation having good height discrimination show no change in angular velocity through the photosphere layers but an increase of 8% for the Hα chromosphere (epoch 1968.9). Spectroscopic results in general are compared with measures made with tracers, i.e. sunspots, filaments, etc., and it is seen that the spectroscopic method always shows increased differential rotation with height, while tracers indicate none. A westward flowing wind is proposed that increases in velocity with height, but produces negligible movement to magnetic regions associated with tracers. © 1969 D. Reidel Publishing Company.

引用

页码：448 / &