Simulations of facular magnetic fields on cool stars
Context. Stellar convection in the presence of magnetic field affects the emergent intensity, as well as the structure and evolution of cool main-sequence dwarfs. Aims.
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Tarduno JA.
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Helioseismic evidence that the solar dynamo originates near the tachocline. [PDF]
Mandal K, Kosovichev AG.
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Energetically expensive dynamo action in Earth's basal magma ocean. [PDF]
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Single-Cell Lineage Trajectory Defines Cyclin-Dependent Kinase Inhibitor-Sensitive Cells-of-Origin in Esophageal Squamous Cell Carcinoma. [PDF]
Ko KP, Zhang J, Jun S, Park JI.
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