电邮这篇文章 Transition from super-alfvenic to sub-alfvenic stellar wind flow passing by an exoplanet, using the example of HD 209458b
- 作者: Belenkaya E.1
-
隶属关系:
- Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics (SINP MSU)
- 期: 卷 101, 编号 3 (2024)
- 页面: 244-249
- 栏目: Articles
- URL: https://journals.rcsi.science/0004-6299/article/view/264858
- DOI: https://doi.org/10.31857/S0004629924030053
- EDN: https://elibrary.ru/KJSTYR
- ID: 264858
如何引用文章
开放存取
##reader.subscriptionAccessGranted##
订阅存取
详细
Depending on the distance of the exoplanet from the central star and on the properties of this star, different regimes of stellar wind flow around it arise. If the exoplanet is at a distance up to the Alfven radius at which the wind speed is equal to the Alfven speed, or the Alfven Mach number MA = 1, then the exoplanet generates Alfven wings. If it is located beyond the Alfven radius, a comet-like magnetosphere appears, like that of the planets of the Solar System. The paper examines how the transition from one flow regime to another can be described on the base of a paraboloid model of the magnetospheric magnetic field using the example of exoplanet HD 209458b.
作者简介
E. Belenkaya
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics (SINP MSU)
编辑信件的主要联系方式.
Email: elena@dec1.sinp.msu.ru
俄罗斯联邦, Moscow
参考
- A. A. Vidotto, M. Jardine, J. Morin, J. F. Donati, P. Lang, and A. Russell, Astron. and Astrophys. 557, id. A67 (2013).
- Y. Vernisse, J.A. Riousset, U. Motschmann, and K.H. Glassmeier, Planet. Space Sci. 137, 40 (2017).
- C. Fischer and J. Saur, Astron. and Astrophys. 668, id. A10 (2022).
- А.Г. Жилкин, Д.В. Бисикало, Астрон. журн. 96(7), 547 (2019).
- А.Г. Жилкин, Д.В. Бисикало, Астрон. журн. 97(7), 538 (2020).
- А.Г. Жилкин, Д.В. Бисикало, П.В. Кайгородов, Астрон. журн. 97(2), 145 (2020).
- E. Chané, J. Saur, F. M. Neubauer, J. Raeder, and S. Poedts, J. Geophys. Res. Space Physics 117(A9), id. A09217 (2012).
- A. J. Ridley, Ann. Geophysicae 25(2), 533 (2007), https://www.ann-geophys.net/25/533/2007.
- K. G. Kislyakova, M. Holmström, H. Lammer, P. Odert, and M. L. Khodachenko, Science 346, 981 (2014).
- J. Nichols and S. E. Milan, Monthly Not. Roy. Astron. Soc. 461, 2353 (2016).
- E.S. Belenkaya, I.I. Alexeev, and M.S. Blokhina, Universe 8, 231 (2022).
- I.I. Alexeev, Moscow University Phys. Bull. 65, 300 (2010).
