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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Ngā kaituhi matua:	Cai Jinshu, Dang Tong, Lei Jiuhou, Zhang Binzheng, Yao Zhonghua, Chen Junjie, Xu Xiaohang, Xiao Sudong, Zhang Tielong
Hōputu:	Artigo
Reo:	Inglês
I whakaputaina:	EDP Sciences 2026-02-01
Rangatū:	Astronomy & Astrophysics
Ngā marau:	magnetohydrodynamics (mhd) methods: numerical planets and satellites: atmospheres planets and satellites: magnetic fields planets and satellites: terrestrial planets
Urunga tuihono:	https://www.aanda.org/articles/aa/full_html/2026/02/aa55227-25/aa55227-25.html
Ngā Tūtohu:	Tāpirihia he Tūtohu Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!