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Reference Work Entry In depth
Core Dynamo
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Article
Open AccessDetermination of the lunar body tide from global laser altimetry data
We use global data from the Lunar Orbiter Laser Altimeter (LOLA) to retrieve the lunar tidal Love number \(h_2\) ...
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Living Reference Work Entry In depth
Core Dynamo
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Article
Global-scale equatorial Rossby waves as an essential component of solar internal dynamics
The Sun’s complex dynamics is controlled by buoyancy and rotation in the convection zone. Large-scale flows are dominated by vortical motions1 and appear to be weaker than expected in the solar interior2. One pos...
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Reference Work Entry In depth
Core Dynamo
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Article
The Earth’s Magnetic Field in the Space Age: An Introduction to Terrestrial Magnetism
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Article
Paleomagnetic Records of Meteorites and Early Planetesimal Differentiation
The large-scale compositional structures of planets are primarily established during early global differentiation. Advances in analytical geochemistry, the increasing diversity of extraterrestrial samples, and...
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Chapter
Paleomagnetic Records of Meteorites and Early Planetesimal Differentiation
The large-scale compositional structures of planets are primarily established during early global differentiation. Advances in analytical geochemistry, the increasing diversity of extraterrestrial samples, and...
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Article
Energy flux determines magnetic field strength of planets and stars
Some planets and many stars have magnetic fields that are generated by a convection-driven dynamo process. Stellar fields, known from their effect on the emitted light, are often 1,000 times stronger than that...
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Article
A sheet-metal geodynamo
A decade of modelling Earth's core on computers has led to the belief that we understand what produces Earth's magnetic field. More realistic simulations are now shaking that complacency.
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Article
A deep dynamo generating Mercury’s magnetic field
The latest numerical models of the geodynamo can account for the behaviour of Earth's magnetic field pretty well: Mercury has proved a harder nut to crack. Like Earth, it has a dipolar magnetic field, probably...
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Article
Power requirement of the geodynamo from ohmic losses in numerical and laboratory dynamos
In the Earth's fluid outer core, a dynamo process converts thermal and gravitational energy into magnetic energy. The power needed to sustain the geomagnetic field is set by the ohmic losses (dissipation due t...
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Article
A one-plume model of martian mantle convection
FOR at least the past two billion years, volcanism on Mars has been restricted to the Tharsis region1. In addition, most tectonic activity on Mars2, together with the long-wavelength topography and the non-hydros...
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Chapter
Mantle Convection with Active Chemical Heterogeneities
The main source of mantle heterogeneity is the subduction of basaltic oceanic crust. Whether or not coherent lumps of continental crust are recycled in significant amounts is unkown. These heterogeneities will...