Response of Venusian plasma environment to the interplanetary coronal mass ejections on 5 November 2011: A magnetohydrodynamics simulation study

Context. As an unmagnetized planet, Venus lacks an intrinsic magnetic field, leading to the direct interaction with the solar wind, which results in differences in physical processes within its magnetosphere–ionosphere (MI) system compared to Earth. With intense solar wind disturbances, it has been...

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Detaylı Bibliyografya
Asıl Yazarlar:	Cai Jinshu, Dang Tong, Lei Jiuhou, Zhang Binzheng, Yao Zhonghua, Chen Junjie, Xu Xiaohang, Xiao Sudong, Zhang Tielong
Materyal Türü:	Artigo
Dil:	Inglês
Baskı/Yayın Bilgisi:	EDP Sciences 2026-02-01
Seri Bilgileri:	Astronomy & Astrophysics
Konular:	magnetohydrodynamics (mhd) methods: numerical planets and satellites: atmospheres planets and satellites: magnetic fields planets and satellites: terrestrial planets
Online Erişim:	https://www.aanda.org/articles/aa/full_html/2026/02/aa55227-25/aa55227-25.html
Etiketler:	Etiketle Etiket eklenmemiş, İlk siz ekleyin!

Response of Venusian plasma environment to the interplanetary coronal mass ejections on 5 November 2011: A magnetohydrodynamics simulation study

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