Probing the Variation with Depth of the Solar Meridional Circulation Using Legendre Function Decomposition

D. C. Braun, A. Birch, Y. Fan

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

We apply the helioseismic methodology of Legendre Function Decomposition to 7.5 years of Dopplergrams obtained by the Helioseismic and Magnetic Imager (HMI) as the basis of inferring the depth variation of the meridional flow between 20◦ and 60◦ latitude in both hemispheres. We assess and remove centerto-limb artifacts using measurements obtained by applying the procedure to pseudo poles at the east and west limbs. Forward modeling is carried out to evaluate the consistency of the corrected frequency shifts with models of the depth variation of the meridional circulation in the top half of the convection zone. The observations are consistent with a return flow in the northern hemisphere below about 40 Mm depth, but no obvious return flow in the south.

Original languageEnglish
Title of host publicationDynamics of the Sun and Stars - Honoring the Life and Work of Michael J. Thompson
EditorsMário J. P. F. G. Monteiro, Rafael A. García, Jørgen Christensen-Dalsgaard, Scott W. McIntosh
PublisherSpringer Science and Business Media B.V.
Pages125-126
Number of pages2
ISBN (Print)9783030553357
DOIs
StatePublished - 2020
EventMeeting celebrating Michael Thompson's seminal work on solar and stellar physics, 2019 - Boulder, United States
Duration: Sep 24 2019Sep 26 2019

Publication series

NameAstrophysics and Space Science Proceedings
Volume57
ISSN (Print)1570-6591
ISSN (Electronic)1570-6605

Conference

ConferenceMeeting celebrating Michael Thompson's seminal work on solar and stellar physics, 2019
Country/TerritoryUnited States
CityBoulder
Period09/24/1909/26/19

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