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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Michael Indergaard,Michael CushionTime-distance helioseismic studies of the deep structure of MC, however, have yielded conflicting inferences. Here, following a summary of existing results we show how a large center-to-limb systematics (CLS) in the measured travel times of acoustic waves affects the inferences through an analysis o

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Developments in Hematology and Immunologyrather easily. Here we show the result of the measurement of rotation periods for a large number of . solar-like stars along with their level of magnetic 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

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Platelet Functions and Platelet Transfusionrted in time–distance helioseismic measurements. Meanwhile, another travel-time asymmetry between waves traveling away from and into sunspots is well known. It is possible that both of the travel-time asymmetries are partially, albeit not entirely, due to different atmospheric heights where oscillat

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https://doi.org/10.1007/978-1-4613-3458-34). Optimization procedures that rely on matrix inversions may suffer from numerical instabilities caused by ill-conditioned matrices. Markov Chain Monte Carlo (MCMC) methods sample the parameter space, independent of its complexity, while Bayesian methods are powerful ways of of understanding the p

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