Time-distance helioseismology with f modes as a method for measurement of near-surface flows

被引：135

作者：

Duvall, TL ^{[1
]}

Gizon, L

机构：

[1] NASA, Goddard Space Flight Ctr, Astron & Solar Phys Lab, Greenbelt, MD 20771 USA

[2] Stanford Univ, WW Hansen Expt Phys Lab, Stanford, CA 94305 USA

来源：

SOLAR PHYSICS | 2000年 / 192卷 / 1-2期

关键词：

D O I：

10.1023/A:1005239503637

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Travel times measured for the f mode have been used to study flows near the solar surface in conjunction with simultaneous measurements of the magnetic field. Previous flow measurements of Doppler surface rotation, small magnetic feature rotation, supergranular pattern rotation, and surface meridional circulation have been confirmed. In addition, the flow in supergranules due to Coriolis forces has been measured. The spatial and temporal power spectra for a six-day observing sequence have been measured.

引用

页码：177 / 191

页数：15

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