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Energy Dissipation in the Upper Atmospheres of Trappist-1 Planets
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...
Tallennettuna:
| Julkaisussa: | Astrophys J Lett |
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| Päätekijät: | , , , , |
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
2018
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| Aiheet: | |
| Linkit: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7493050/ https://ncbi.nlm.nih.gov/pubmed/32944211 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.3847/2041-8213/aab5b5 |
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