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Constraining the Ionospheric Impacts of Exoplanet Host Star Emission
2021
Zenodo
We employ a surface flux transport (SFT) model in order to simulate the detailed magnetic structure and dynamics of exoplanet host star photospheres. In coupling the SFT model with a potential-field source surface (PFSS) extrapolation of coronal field, and with a suite of forward-modeling tools for the derivation of coronal X-ray and EUV emission, we simulate self-consistently the magnetic structure and energetic budget of host star surfaces and coronae. In particular, our modeling framework
doi:10.5281/zenodo.4567672
fatcat:tm4bixwed5akhklb6ns54wbhva