Corpus ID: 237428072

Corona and XUV emission modelling of the Sun and Sun-like stars

@inproceedings{Shoda2021CoronaAX,
  title={Corona and XUV emission modelling of the Sun and Sun-like stars},
  author={M. Shoda and S. Takasao},
  year={2021}
}
The X-ray and extreme-ultraviolet (EUV) emissions from the low-mass stars significantly affect the evolution of the planetary atmosphere. However, it is, observationally difficult to constrain the stellar high-energy emission because of the strong interstellar extinction of EUV photons. In this study, we simulate the XUV (X-ray+EUV) emission from the Sun-like stars by extending the solar coronal heating model that self-consistently solves, with sufficiently high resolution, the surface-to… Expand

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A&A proofs: manuscript no. main
    Corona and XUV emission modelling of the Sun and Sun-like stars