Enviar artigo por via de e-mail INTERACTION OF THE EXOPLANET HAT–P–11b WITH THE STELLAR WIND
- Autores: Belenkaya E.1
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Afiliações:
- Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics (SINP MSU)
- Edição: Volume 100, Nº 11 (2023)
- Páginas: 958-963
- Seção: Articles
- URL: https://journals.rcsi.science/0004-6299/article/view/148083
- DOI: https://doi.org/10.31857/S0004629923110026
- EDN: https://elibrary.ru/AGTVHH
- ID: 148083
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Resumo
This article discusses the possibility of the existence of a magnetodisk around the exoplanet HAT–P–11b. We used the available observational data to determine the properties of this exoplanet and the stellar wind passing by it, and obtained a rough estimate of the planetary magnetospheric scale. Our estimate was compared with the published results of calculations by the Particle-In-Cell method in a three-dimensional electromagnetic relativistic collisionless model of the magnetosphere. The resulting discrepancy between the magnetospheric scales obtained by these two methods is discussed, and its possible interpretation is proposed.
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Sobre autores
E. Belenkaya
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics (SINP MSU)
Autor responsável pela correspondência
Email: elena.belenkaya.msu@gmail.com
Russia, Moscow
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