Plasma Environment, Radiation, Structure, and Evolution of the Uranian System (PERSEUS): A Dedicated Orbiter Mission Concept to Study Space Physics at Uranus. [PDF]
Space Sci Rev, 2023 Cohen IJ +13 more
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Uranus' Complex Internal Structure
Uranus' bulk composition remains unknown. Although there are clear indications that Uranus' interior is not fully convective, and therefore has a non-adiabatic temperature profile, many interior models continue to assume an adiabatic interior.
Neuenschwander, Benno A. +2 more
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Double superionicity in icy compounds at planetary interior conditions. [PDF]
Nat Commun, 2023 de Villa K +2 more
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Magnesium oxide-water compounds at megabar pressure and implications on planetary interiors. [PDF]
Nat Commun, 2023 Pan S +9 more
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Deuterated water and the formation of the satellites of Uranus. [PDF]
Proc Natl Acad Sci U S ABrown ME +7 more
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Seeking answers, planetary scientists plot a return to the nearest ice giant. [PDF]
Proc Natl Acad Sci U S A, 2022 Croswell K.
europepmc +1 more source
Neuroendoscopy-assisted drainage versus burr hole drainage for chronic subdural hematoma (URANUS): study protocol for a multicenter randomized controlled trial. [PDF]
TrialsWu L +6 more
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Plastic deformation of superionic water ices. [PDF]
Proc Natl Acad Sci U S A, 2022 Matusalem F, Santos Rego J, de Koning M.
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Photochemical Haze Formation on Titan and Uranus: A Comparative Review. [PDF]
Int J Mol SciDubois D.
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Magneto-hydrostatic equilibrium configurations for the magnetosphere of Uranus
, 1984 Text includes handwritten formulasAt the time of the Voyager 2 flyby of Uranus, the rotational axis of the planet will be roughly antiparallel to the solar wind flow. If Uranus has a magnetic dipole moment that is approximately aligned with its spin axis,
Ip, Antonio K.
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