Improved Helioseismic Analysis of Medium-l Data from the Michelson Doppler Imager
Tim Larson, Jesper Schou

TL;DR
This paper improves helioseismic analysis methods using MDI data, leading to more accurate measurements of solar oscillation modes and insights into the Sun's internal rotation.
Contribution
It introduces updated data processing techniques and physical effect considerations, significantly enhancing the accuracy of global-mode parameter estimation from helioseismic data.
Findings
Significant changes in mode parameters due to processing updates
Reduced residuals in internal rotation inversions
Detection of an annual periodicity in f-mode frequencies
Abstract
We present a comprehensive study of one method for measuring various parameters of global modes of oscillation of the Sun. Using velocity data taken by the Michelson Doppler Imager (MDI), we analyze spherical harmonic degrees l <= 300. Both current and historical methodologies are explained, and the various differences between the two are investigated to determine their effects on global-mode parameters and systematic errors in the analysis. These differences include a number of geometric corrections made during spherical harmonic decomposition; updated routines for generating window functions, detrending timeseries, and filling gaps; and consideration of physical effects such as mode profile asymmetry, horizontal displacement at the solar surface, and distortion of eigenfunctions by differential rotation. We apply these changes one by one to three years of data, and then reanalyze the…
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