Helioseismic Inversion to Infer the Depth Profile of Solar Meridional Flow Using Spherical Born Kernels
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/863/i=1/a=39/pdf
Reference34 articles.
1. EFFECTS OF ASYMMETRIC FLOWS IN SOLAR CONVECTION ON OSCILLATION MODES
2. CHARACTERISTICS OF SOLAR MERIDIONAL FLOWS DURING SOLAR CYCLE 23
3. Ring Diagram Analysis of Near‐Surface Flows in the Sun
4. Recovery of subsurface profiles of supergranular flows via iterative inversion of synthetic travel times
5. Accuracy of the Born and Ray Approximations for Time‐Distance Helioseismology of Flows
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