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      Oceans in the icy Galilean satellites of Jupiter?

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      Icarus
      Elsevier BV

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          Scaling of temperature‐ and stress‐dependent viscosity convection

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            Galileo magnetometer measurements: a stronger case for a subsurface ocean at Europa.

            On 3 January 2000, the Galileo spacecraft passed close to Europa when it was located far south of Jupiter's magnetic equator in a region where the radial component of the magnetospheric magnetic field points inward toward Jupiter. This pass with a previously unexamined orientation of the external forcing field distinguished between an induced and a permanent magnetic dipole moment model of Europa's internal field. The Galileo magnetometer measured changes in the magnetic field predicted if a current-carrying outer shell, such as a planet-scale liquid ocean, is present beneath the icy surface. The evidence that Europa's field varies temporally strengthens the argument that a liquid ocean exists beneath the present-day surface.
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              Superplastic deformation of ice: Experimental observations

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                Author and article information

                Journal
                Icarus
                Icarus
                Elsevier BV
                00191035
                February 2003
                February 2003
                : 161
                : 2
                : 456-467
                Article
                10.1016/S0019-1035(02)00048-9
                89fa363f-be6c-48cf-a5b4-ad7313dcd96f
                © 2003

                http://www.elsevier.com/tdm/userlicense/1.0/

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