How Much Data Do We Need to Detect the Deep Solar Meridional Circulation?

Details How Much Data Do We Need to Detect the Deep Solar Meridional Circulation? How Much Data Do We Need to Detect the Deep Solar Meridional Circulation?

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..416..131b&link_type=abstract

Solar-Stellar Dynamos as Revealed by Helio- and Asteroseismology: GONG 2008/SOHO 21 ASP Conference Series, Vol. 416, proceedings

Astronomy and Astrophysics

Astronomy

Scientific paper

We assess the noise in p-mode travel-time shifts which would form the basis of inferences of large-scale flows throughout the solar convection zone. We derive the expected travel times from a parameterized return flow component of the meridional circulation. We show that a helioseismic detection of the return component may not be possible using data spanning an interval less than a solar cycle.

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