Titlebook: Dynamics of the Sun and Stars; Honoring the Life an Mário J. P. F. G. Monteiro,Rafael A. García,Scott Conference proceedings 2020 The Edit

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https://doi.org/10.1007/978-1-4612-5248-1cument. Dynamics of the Sun & Stars: Honoring the Life & Work of Michael Thompson was a wonderful gathering of Michael’s family, friends and colleagues to discuss the science that was his passion and to commemorate his many professional achievements.

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Workers, Managers, and Technological Changervations but which helioseismology reveals to penetrate deep into the convection zone. Finally, I briefly mention the collaborative effort that was initiated by Michael in 2017 with the aim of taking advantage of more than twenty years of high-quality helioseismic observations to refine our picture of the interior rotation profile.

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Surface Rotation and Magnetic Activity of Solar-Like Stars: Impact on Seismic Detectionstic activity. We also study solar-like stars for which oscillations have not been detected using 1 month of . data in order to understand what can be the reason behind these non-detections. Surprisingly the conclusion of our analysis is that magnetic activity is not the main reason for not detecting acoustic modes in those stars.

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Michael Indergaard,Michael Cushionf frequency dependence of CLS, using data from the Helioseismic and Doppler Imager (HMI) onboard Solar Dynamics Observatory (SDO). Our results point to the residual systematics in travel times as a major cause of differing inferences on the deep structure of MC.