Abstract
We present the results of new global 3D MHD simulations of early M-Dwarf stars, exploring the influence that a tachocline of shear has on their instantaneous and long-term magnetic activity.
This work funded by NASA ATP grant NNX17AG22G.
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Bice, C., Toomre, J. (2020). Exploring the Origins of Intense Magnetism in Early M-Dwarf Stars. In: Monteiro, M.J.P.F.G., GarcÃa, R.A., Christensen-Dalsgaard, J., McIntosh, S.W. (eds) Dynamics of the Sun and Stars. Astrophysics and Space Science Proceedings, vol 57. Springer, Cham. https://doi.org/10.1007/978-3-030-55336-4_40
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DOI: https://doi.org/10.1007/978-3-030-55336-4_40
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