Modeling the young Sun's solar wind and its interaction with Earth's paleomagnetosphere

We present a focused parameter study of solar wind–magnetosphere interaction for the young Sun and Earth, ∼3.5 Gyr ago, that relies on magnetohydrodynamic (MHD) simulations for both the solar wind and the magnetosphere. By simulating the quiescent young Sun and its wind we are able to propagate the...

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Veröffentlicht in:	Journal of Geophysical Research: Space Physics 2011-01, Vol.116 (A1), p.n/a
Hauptverfasser:	Sterenborg, M. Glenn, Cohen, O., Drake, J. J., Gombosi, T. I.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Astrophysics Atmospheric evolution Atmospheric sciences Earth Earth sciences Earth, ocean, space Exact sciences and technology Geological time Magnetic fields Magnetism MHD simulation paleomagnetosphere Physics solar wind Sun Wind speed young Sun
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