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Title:
Latest Results Found with Ring-Diagram Analysis
Authors:
Baldner, C. S.; Basu, S.; Bogart, R. S.; Burtseva, O.; González Hernández, I.; Haber, D.; Hill, F.; Howe, R.; Jain, K.; Komm, R. W.; Rabello-Soares, M. C.; Tripathy, S.
Affiliation:
AA(Hansen Experimental Physics Laboratory, Stanford University), AB(Department of Astronomy, Yale University), AC(Hansen Experimental Physics Laboratory, Stanford University), AD(National Solar Observatory), AE(National Solar Observatory), AF(JILA, University of Colorado), AG(National Solar Observatory), AH(School of Physics and Astronomy, University of Birmingham), AI(National Solar Observatory), AJ(National Solar Observatory), AK(Department of Physics, Universidade Federal de Minas Gerais), AL(National Solar Observatory)
Publication:
Solar Physics, Volume 287, Issue 1-2, pp. 57-69 (SoPh Homepage)
Publication Date:
10/2013
Origin:
SPRINGER
Keywords:
Helioseismology, Observations
Abstract Copyright:
(c) 2013: Springer Science+Business Media Dordrecht
DOI:
10.1007/s11207-012-0171-x
Bibliographic Code:
2013SoPh..287...57B

Abstract

Ring-diagram analysis is a helioseismic tool useful for studying the near-surface layers of the Sun. It has been employed to study near-surface shear, meridional circulation, flows around sunspots, and thermal structure beneath active regions. We review recent results obtained using ring-diagram analysis, state some of the more important outstanding difficulties in the technique, and point out several extensions to the technique that are just now beginning to bear fruit.
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Database: Astronomy
Physics
arXiv e-prints