Characterizing the Magnetic Environment of Exoplanet Stellar Systems

  title={Characterizing the Magnetic Environment of Exoplanet Stellar Systems},
  author={Alison O. Farrish and David Alexander and Mei Maruo and M. L. DeRosa and Frank R. Toffoletto and Anthony Sciola},
  journal={The Astrophysical Journal},
2 Citations
Modeling Stellar Activity-rotation Relations in Unsaturated Cool Stars
We apply a surface flux transport model developed for the Sun to reconstruct the stellar activity-rotation relationship, L X /L bol versus Ro, observed for unsaturated cool stars (Rossby numbers Ro ≳


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The combination of high-contrast imaging and high-dispersion spectroscopy, which has successfully been use to detect the atmosphere of a giant planet, is one of the most promising potential probes of
Asteroseismology and Exoplanets: Listening to the Stars and Searching for New Worlds
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Effect of Magnetic Field Strength on Solar Differential Rotation and Meridional Circulation.
We studied the solar surface flows (differential rotation and meridional circulation) using a magnetic element feature tracking technique by which the surface velocity is obtained using magnetic
Observing the simulations: applying ZDI to 3D non-potential magnetic field simulations
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The Revolution Revolution: Magnetic Morphology Driven Spin-down
Observations of young open clusters show a bimodal distribution of rotation periods that has been difficult to explain with existing stellar spin-down models. Detailed MHD stellar wind simulations