Magnetization of sinking porous diapirs in planetesimal cores
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[1] D. Bercovici,et al. Two-phase magnetohydrodynamics: Theory and applications to planetesimal cores , 2020 .
[2] C. Russell,et al. Observations, Meteorites, and Models: A Preflight Assessment of the Composition and Formation of (16) Psyche , 2020, Journal of geophysical research. Planets.
[3] F. Nimmo,et al. The Top‐Down Solidification of Iron Asteroids Driving Dynamo Evolution , 2019, Journal of geophysical research. Planets.
[4] T. Spohn,et al. Top-down freezing in a Fe–FeS core and Ganymede’s present-day magnetic field , 2018, Icarus.
[5] R. Harrison,et al. Paleomagnetic evidence for dynamo activity driven by inward crystallisation of a metallic asteroid , 2017 .
[6] R. Harrison,et al. Magnetic Mineralogy of Meteoritic Metal: Paleomagnetic Evidencefor Dynamo Activity on Differentiated Planetesimals , 2017 .
[7] H. Terasaki. Physical Properties of the Outer Core , 2016 .
[8] D. Bercovici,et al. Core solidification and dynamo evolution in a mantle‐stripped planetesimal , 2016 .
[9] T. Spohn,et al. Iron snow, crystal floats, and inner-core growth: modes of core solidification and implications for dynamos in terrestrial planets and moons , 2015, Progress in Earth and Planetary Science.
[10] T. Spohn,et al. The Fe snow regime in Ganymede's core: A deep‐seated dynamo below a stable snow zone , 2015 .
[11] E. A. Lima,et al. Decline of the lunar core dynamo , 2014 .
[12] Linda T. Elkins-Tanton,et al. Differentiated Planetesimals and the Parent Bodies of Chondrites , 2013 .
[13] J. Head,et al. Persistence and origin of the lunar core dynamo , 2013, Proceedings of the National Academy of Sciences.
[14] R. Secco. Viscosity of the Outer Core , 2013 .
[15] Q. Williams. Bottom-up versus top-down solidification of the cores of small solar system bodies: Constraints on paradoxical cores , 2009 .
[16] F. Nimmo. Energetics of asteroid dynamos and the role of compositional convection , 2009 .
[17] E. A. Lima,et al. Magnetism on the Angrite Parent Body and the Early Differentiation of Planetesimals , 2008, Science.
[18] T. Alboussière,et al. On the existence and structure of a mush at the inner core boundary of the Earth , 2007, 0801.2897.
[19] S. Hauck,,et al. Sulfur's impact on core evolution and magnetic field generation on Ganymede , 2005 .
[20] J. Goff. Heuristic model of air drag on a sphere , 2004 .
[21] M. Kivelson,et al. The Permanent and Inductive Magnetic Moments of Ganymede , 2002 .
[22] P. Davidson. An Introduction to Magnetohydrodynamics , 2001 .
[23] Ulrich R. Christensen,et al. Numerical modelling of the geodynamo: a systematic parameter study , 1999 .
[24] M. Manga. Interactions between mantle diapirs , 1997 .
[25] D. J. Southwood,et al. Discovery of Ganymede's magnetic field by the Galileo spacecraft , 1996, Nature.
[26] Rainer Hollerbach. ON THE THEORY OF THE GEODYNAMO , 1996 .
[27] M. Manga. Waves of bubbles in basaltic magmas and lavas , 1996 .
[28] H. Power,et al. Integral-equation solution of potential flow past a porous body of arbitrary shape , 1984, Journal of Fluid Mechanics.
[29] G. Batchelor,et al. An Introduction to Fluid Dynamics , 1968 .
[30] Richard Van Blerkom. Magnetohydrodynamic flow of a viscous fluid past a sphere , 1960, Journal of Fluid Mechanics.
[31] I. Sumita,et al. Inner core dynamics , 2022, Earth's Core.
[32] Linda T. Elkins-Tanton,et al. Magnetic fields on asteroids and planetesimals , 2017 .
[33] J. Crowley,et al. Thermal evolution of early solar system planetesimals and the possibility of sustained dynamos , 2013 .
[34] M. Grae Worster,et al. CONVECTION IN MUSHY LAYERS , 1997 .
[35] Raymond A. Serway,et al. Printed test bank to accompany Physics for scientists and engineers with modern physics , 1982 .