37 research outputs found
Stellar Coronal and Wind Models: Impact on Exoplanets
Full text linkSurface magnetism is believed to be the main driver of coronal heating and
stellar wind acceleration. Coronae are believed to be formed by plasma confined
in closed magnetic coronal loops of the stars, with winds mainly originating in
open magnetic field line regions. In this Chapter, we review some basic
properties of stellar coronae and winds and present some existing models. In
the last part of this Chapter, we discuss the effects of coronal winds on
exoplanets.Comment: Chapter published in the "Handbook of Exoplanets", Editors in Chief:
Juan Antonio Belmonte and Hans Deeg, Section Editor: Nuccio Lanza. Springer
Reference Work
Due Process, Fair Play, and Excessive Partisanship: A New Principle for Judicial Review of Election Laws
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Prior Restraints and Intellectual Property: The Clash Between Intellectual Property and the First Amendment From an Economic Perspective
No full textThe Praetorians: An Analysis of U.S. Border Patrol Checkpoints Following Martinez-Fuerte
No full textInterpreting the Qur'an and the Constitution: Similarities in the Use of Text, Tradition, and Reason in Islamic and American Jurisprudence
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