Saturn’s high degree magnetic moments: Evidence for a unique planetary dynamo
暂无分享,去创建一个
[1] C. Russell,et al. Saturn's very axisymmetric magnetic field: No detectable secular variation or tilt , 2011 .
[2] Ulrich R. Christensen,et al. Dynamo Scaling Laws and Applications to the Planets , 2010 .
[3] C. Guervilly,et al. Numerical simulations of dynamos generated in spherical Couette flows , 2010, 1010.3859.
[4] S. Stanley. A dynamo model for axisymmetrizing Saturn's magnetic field , 2010 .
[5] S. M. Krimigis,et al. Particle pressure, inertial force, and ring current density profiles in the magnetosphere of Saturn, based on Cassini measurements , 2010 .
[6] Ronald Redmer,et al. Demixing of hydrogen and helium at megabar pressures. , 2009, Physical review letters.
[7] D. Ceperley,et al. Phase separation in hydrogen–helium mixtures at Mbar pressures , 2009, Proceedings of the National Academy of Sciences.
[8] U. Christensen,et al. Energy flux determines magnetic field strength of planets and stars , 2009, Nature.
[9] U. Christensen,et al. Models of magnetic field generation in partly stable planetary cores: Applications to Mercury and Saturn , 2008 .
[10] Emma J. Bunce,et al. Cassini observations of the variation of Saturn's ring current parameters with system size , 2007 .
[11] U. Christensen,et al. Scaling properties of convection-driven dynamos in rotating spherical shells and application to planetary magnetic fields , 2006 .
[12] N Achilleos,et al. Cassini Magnetometer Observations During Saturn Orbit Insertion , 2005, Science.
[13] Ulrich R. Christensen,et al. Power requirement of the geodynamo from ohmic losses in numerical and laboratory dynamos , 2004, Nature.
[14] J. Fortney,et al. Effects of Helium Phase Separation on the Evolution of Extrasolar Giant Planets , 2003, astro-ph/0402620.
[15] Rainer Hollerbach. Instabilities of the Stewartson layer Part 1. The dependence on the sign of $Ro$ , 2003, Journal of Fluid Mechanics.
[16] Johannes Wicht. Inner-core conductivity in numerical dynamo simulations , 2002 .
[17] J. Aurnou,et al. A polar vortex in the Earth's core , 1999, Nature.
[18] W. J. Nellis,et al. Metallization of fluid molecular hydrogen at 140 GPa (1.4 Mbar) , 1996 .
[19] Edward J. Smith,et al. A model of Saturn's magnetic field based on all available data , 1990 .
[20] J. Connerney,et al. Magnetic Field Studies by Voyager 2: Preliminary Results at Saturn , 1982, Science.
[21] J. Connerney,et al. Magnetic field studies by voyager 1: preliminary results at saturn. , 1981, Science.
[22] D. Stevenson,et al. Saturn's Luminosity and Magnetism , 1980, Science.
[23] E. Smith,et al. Saturn's Magnetic Field and Magnetosphere , 1980, Science.
[24] C. Russell,et al. On the apparent source depth of planetary magnetic fields , 1978 .
[25] D. Stevenson. Thermodynamics and phase separation of dense fully ionized hydrogen-helium fluid mixtures , 1975 .
[26] F. Lowes,et al. Spatial Power Spectrum of the Main Geomagnetic Field, and Extrapolation to the Core , 1974 .
[27] K. Stewartson. On almost rigid rotations. Part 2 , 1966, Journal of Fluid Mechanics.
[28] T. G. Cowling,et al. The Magnetic Field of Sunspots , 1933 .
[29] Ulrich R. Christensen,et al. Numerical Dynamo Simulations , 2007 .
[30] D. Stevenson. Reducing the non-axisymmetry of a planetary dynamo and an application to saturn , 1982 .