A new estimate of the solar meridional flow

被引：20

作者：

Cameron, R ^{[1
]}

Hopkins, A ^{[1
]}

机构：

[1] Univ Sydney, Sch Math & Stat, Sydney, NSW 2006, Australia

来源：

SOLAR PHYSICS | 1998年 / 183卷 / 02期

基金：

美国国家科学基金会; 美国国家航空航天局;

关键词：

D O I：

10.1023/A:1005036907969

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a new method for measuring the solar magnetic meridional flow, and provide a comparison with other recent work. We have performed a least-squares fit to azimuthally averaged Mount Wilson Observatory synoptic data encompassing Carrington rotations 1722 to 1929 to produce an estimate of the solar meridional flow. A parametric fit to our results expresses the solar meridional flow as nu(phi) = 28.5 sin(2.5) phi cos phi.

引用

页码：263 / 276

页数：14

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