Email this article Modeling of the exoplanet HAT-P-11b magnetosphere
- Authors: Belenkaya E.S.1, Alexeev I.I.1, Kalegaev V.V.1
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Affiliations:
- Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics (SINP MSU)
- Issue: Vol 101, No 1 (2024)
- Pages: 25-33
- Section: Articles
- URL: https://journals.rcsi.science/0004-6299/article/view/261214
- DOI: https://doi.org/10.31857/S0004629924010031
- EDN: https://elibrary.ru/LFUZWY
- ID: 261214
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Abstract
Based on the available data on the magnetic field of the star HAT-P-11 and its closest exoplanet HAT-P-11b, as well as information on the stellar wind in this system, we construct the HAT-P-11b magnetic field magnetospheric model. We show how the value and orientation of the interplanetary magnetic field control the magnetospheric structure. Each component of the stellar wind’s magnetic field creates a specific type of reconnection with the exoplanet’s magnetic field.
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About the authors
E. S. Belenkaya
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics (SINP MSU)
Author for correspondence.
Email: elena@dec1.sinp.msu.ru
Russian Federation, Moscow
I. I. Alexeev
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics (SINP MSU)
Email: iialexeev@mail.ru
Russian Federation, Moscow
V. V. Kalegaev
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics (SINP MSU)
Email: klg@dec1.sinp.msu.ru
Russian Federation, Moscow
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