Astronomy and Astrophysics – Astronomy
Scientific paper
May 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011spd....42.1608b&link_type=abstract
American Astronomical Society, SPD meeting #42, #16.08; Bulletin of the American Astronomical Society, Vol. 43, 2011
Astronomy and Astrophysics
Astronomy
Scientific paper
Ring diagrams are used to study the structure and dynamics of the near-surface layers of the Sun. The parameters of primary interest are frequencies and velocities in both the zonal and merridional direction as a function of wavenumber and of radial order n. These parameters are recovered by fitting a model of the spectral profile to three-dimensional power spectra of small regions of the Sun. In this work, we examine the systematic differences between fits assuming an asymmetric profile and fits assuming a symmetric profile. We also explore the coupling between the parameters of interest and certain secondary parameters such as amplitude, width, and asymmetry.
Baldner Charles
Basu Sarbani
Bogart Rick
Haber Deborah
Hill F. F.
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