ArticleThe astrophysical journal. Letters2018
Energy Dissipation in the Upper Atmospheres of Trappist-1 Planets.
Article in The astrophysical journal. Letters, 2018. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 2 papers.
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2 citing papers in PubMed, 25 citations in OpenAlex.
- Modeling a Carrington-scale Stellar Superflare and Coronal Mass Ejection fromThe Astrophysical journal · 2019Article
- EXOPLANET MODULATION OF STELLAR CORONAL RADIO EMISSION.The Astronomical journal · 2018Article
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Authors and funding
5 authors at 4 institutions in 1 country.
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Abstract
We present a method to quantify the upper-limit of the energy transmitted from the intense stellar wind to the upper atmospheres of three of the Trappist-1 planets (e, f, and g). We use a formalism that treats the system as two electromagnetic regions, where the efficiency of the energy transmission between one region (the stellar wind at the planetary orbits) to the other (the planetary ionospheres) depends on the relation between the conductances and impedances of the two regions. Since the energy flux of the stellar wind is very high at these planetary orbits, we find that for the case of high transmission efficiency (when the conductances and impedances are close in magnitude), the energy dissipation in the upper planetary atmospheres is also very large. On average, the Ohmic energy can reach 0.5 - 1
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