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Solar Internal Rotation

Published online by Cambridge University Press:  08 February 2017

Jesper Schou  and
The SOI Internal Rotation team
Jesper Schou
Affiliation:
HEPL Annex A201, Stanford, CA 94305-4085, USA
The SOI Internal Rotation team
Affiliation:
HEPL Annex A201, Stanford, CA 94305-4085, USA

Abstract

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With the flood of high quality helioseismic data from the instruments on the SOHO spacecraft (MDI/VIRGO/GOLF) and ground based instruments (e.g. GONG, LOWL, BiSON, IRIS, MWO-CrAO and TON) we have been able to get increasingly detailed information on the rotation and other large scale flows in the solar interior.

Here we will discuss some of the highlights of what we have learned so far and what we may expect to learn in the near future. Among the recent advances have been tighter constraints on the tachocline at the bottom of the convection zone and detection of details in the surface rotation rate similar to the torsional oscillations found in the surface Doppler shift.

Type
III. Large-Scale Structure of the Sun
Information
Symposium - International Astronomical Union , Volume 185: New Eyes to See Inside the Sun and Stars , 1998 , pp. 141 - 148
Copyright
Copyright © Kluwer 1998 

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