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Modeling of Magnetospheres of Terrestrial Exoplanets in the Habitable Zone around G-Type Stars. UNIVERSE 2022. [DOI: 10.3390/universe8040231] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/16/2022]
Abstract
Using a paraboloid model of an Earth-like exoplanetary magnetospheric magnetic field, developed from a model of the Earth, we investigate the magnetospheric structure of planets located in the habitable zone around G-type stars. Different directions of the stellar wind magnetic field are considered and the corresponding variations in the magnetospheric structure are obtained. It is shown that the exoplanetary environment significantly depends on stellar wind magnetic field orientation and that the parameters of magnetospheric current systems depend on the distance to the stand-off magnetopause point.
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Modeling the Field of the Global Magnetopause. ACTA ACUST UNITED AC 2013. [DOI: 10.1029/gm090p0045] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register]
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Alexeev II, Belenkaya ES, Kalegaev VV, Feldstein YI, Grafe A. Magnetic storms and magnetotail currents. ACTA ACUST UNITED AC 1996. [DOI: 10.1029/95ja03509] [Citation(s) in RCA: 150] [Impact Index Per Article: 5.4] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
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