Magnetohydrodynamic simulations of a uranus-at-equinox type rotating magnetosphere

HIGHLIGHTS

  • who: Griton L. and Pantellini F. from the Institut Recherche en Astrophysique et Planétologie (IRAP), CNRS, CNES, Toulouse, UPS, Toulouse, France have published the research: Magnetohydrodynamic simulations of a Uranus-at-equinox type rotating magnetosphere, in the Journal: (JOURNAL)
  • what: The authors simulate the magnetosphere of fictitious Uranus-like planet plunged in supersonic plasma (the stellar wind) at equinox. simulation with zero wind velocity is also presented to help disentangle the effects of the rotation from the effects of the supersonic wind in the structuring of the planetary magnetic tail. The aim of the . . .

     

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