Mass, energy, and momentum capture from stellar winds by magnetized and unmagnetized planets: implications for atmospheric erosion and habitability-Reference-Cited by-同舟云学术

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Mass, energy, and momentum capture from stellar winds by magnetized and unmagnetized planets: implications for atmospheric erosion and habitability

Published:2018-10-01 Issue:4 Volume:481 Page:5146-5155
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Blackman Eric G¹²³,Tarduno John A¹³

Affiliation:

1. Department of Physics and Astronomy, University of Rochester, Rochester NY 14627, USA

2. Laboratory for Laser Energetics, University of Rochester, Rochester NY 14623, USA

3. Department of Earth and Environmental Sciences, University of Rochester, Rochester NY 14627, USA

Funder

National Science Foundation

Simons Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/481/4/5146/26000905/sty2640.pdf

Reference60 articles.

1. Minimalist coupled evolution model for stellar X-ray activity, rotation, mass loss, and magnetic field

2. Scaling of asymmetric magnetic reconnection: General theory and collisional simulations

3. The independency of stellar mass-loss rates on stellar X-ray luminosity and activity level based on solar X-ray flux and solar wind observations

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