Improving Leakage Matrix Calculation

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

Previous work has revealed discrepancies between the analysis of MDI full disk data and medium-l data from the same time period. Most notably, the full disk analysis lacks some systematic errors and generally results in better fits to the data. One of the differences between the two analyses is the leakage matrix used in the peakbagging. In this poster we discuss the effect of such things as proper pixel integration, higher resolution spherical harmonics, improved interpolation in the remapping, and various point spread functions on the leakage matrix itself and the resulting mode parameters. This work has been supported by NASA contract NAS5-02139.

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