Journal ArticleDOI
The Angular Momentum of the Solar Wind
Edmund J. Weber,Leverett Davis +1 more
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Steady state model of solar wind flow in equatorial plane solved for radial and azimuthal motions, taking into account pressure gradient, magnetic field and gravitational effects as discussed by the authors.Abstract:
Steady state model of solar wind flow in equatorial plane solved for radial and azimuthal motions, taking into account pressure gradient, magnetic field and gravitational effectsread more
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Journal ArticleDOI
Effects of mesh topology on MHD solution features in coronal simulations
TL;DR: In this article , the authors discuss and trade off two main mesh topologies when applied to global solar corona simulations using the unstructured ideal magnetohydrodynamic solver from the COOLFluiD platform.
Book ChapterDOI
Stellar magnetic fields, origin and structure
TL;DR: In this paper, a simple model for the external magnetic field has both a wind zone and a corotating dead zone; the predicted rotational history of the star is discussed, and some support for the model noted from observations of a young, rapidly rotating dwarf star.
Journal ArticleDOI
The Mean Magnetic Field Strength of CI Tau
Kimberly R. Sokal,Christopher M. Johns-Krull,Gregory N. Mace,Larissa Nofi,Lisa Prato,Jae-Joon Lee,Daniel T. Jaffe +6 more
TL;DR: In this article, a blind comparison of two methods to measure the mean surface magnetic field strength of the classical T Tauri star CI Tau based on Zeeman broadening of sensitive spectral lines is presented.
Journal ArticleDOI
Asteroseismic Analysis of α Cen B: Preliminary Tests of Effects of Rotation and Interior Magnetic Field in the Solar-like Star
TL;DR: In this article, the effects of rotation and interior magnetic field during the lifetime of a star were taken into consideration and the model of a Cen B was reconstructed to satisfy the latest non-asteroseismic and asterosityismic observational constraints.