Мақаланы E-mail арқылы жіберу INTERACTION OF THE EXOPLANET HAT–P–11b WITH THE STELLAR WIND
- Авторлар: Belenkaya E.1
-
Мекемелер:
- Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics (SINP MSU)
- Шығарылым: Том 100, № 11 (2023)
- Беттер: 958-963
- Бөлім: 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
Дәйексөз келтіру
Ашық рұқсат
Рұқсат берілді
Тек жазылушылар үшін
Аннотация
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.
Негізгі сөздер
Авторлар туралы
E. Belenkaya
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics (SINP MSU)
Хат алмасуға жауапты Автор.
Email: elena.belenkaya.msu@gmail.com
Russia, Moscow
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