Abstract
We discuss how recent advances in observations, theory and numerical simulations have allowed the stellar community to progress in its understanding of stellar convection, rotation and magnetism and to assess the degree to which the Sun and other stars share similar dynamical properties. Ensemble asteroseismology has become a reality with the advent of large time domain studies, especially from space missions. This new capability has provided improved constraints on stellar rotation and activity, over and above that obtained via traditional techniques such as spectropolarimetry or CaII H&K observations. New data and surveys covering large mass and age ranges have provided a wide parameter space to confront theories of stellar magnetism. These new empirical databases are complemented by theoretical advances and improved multi-D simulations of stellar dynamos. We trace these pathways through which a lucid and more detailed picture of magnetohydrodynamics of solar-like stars is beginning to emerge and discuss future prospects.
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Notes
Note however that such choice of characteristic velocity scale is subject to caution in stellar turbulent convective envelopes that usually possess very large Rm.
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Acknowledgements
This work was partly supported by ERC STARS2 207430 grant, ANR Toupies and IDEE grants, FP7 IRSES 269194 and SPACEINN 312844 programs, INSU/PNST. Funding for the Stellar Astrophysics Centre is provided by The Danish National Research Foundation (Grant agreement no.: DNRF106). The research is supported by the ASTERISK project (ASTERoseismic Investigations with SONG and Kepler) funded by the European Research Council (Grant agreement no.: 267864). CESSI is supported by the Ministry of Human Resource Development, Government of India and IISER Kolkata. A.S.B and R.A.G. acknowledge support by the CNES via GOLF, CoRoT and Solar Orbiter grants. D.N. acknowledges support from the Ramanujan Fellowship (Department of Science and Technology) and a grant from the (United States) Asian Office of Aerospace Research and Development. A.S. Brun is grateful to both the University of Kyoto, RIMS and Prof. M. Yamada, K. Shibata, H. Isobe & S. Takahiro for their invitation in Fall 2013 and to the University of California at Santa Barbara, KITP and the organisers of the waves and flow program in Spring 2014 where most of this paper was written.
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Brun, A.S., García, R.A., Houdek, G. et al. The Solar-Stellar Connection. Space Sci Rev 196, 303–356 (2015). https://doi.org/10.1007/s11214-014-0117-8
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DOI: https://doi.org/10.1007/s11214-014-0117-8