Results 31 to 40 of about 1,386 (209)
Prandtl-number dependence of convection-driven dynamos in rotating spherical fluid shells [PDF]
The value of the Prandtl number P exerts a strong influence on convection-driven dynamos in rotating spherical shells filled with electrically conducting fluids.
Simitev, R., Busse, F.H.
core +1 more source
NUMERICAL SIMULATION IN LOW MODED GEODYNAMOMODEL APPLYING THE PACKAGES OF HIGH PRECISION CALCULATION [PDF]
The means of high precision calculation are considered, their comparative analysis isfulfilled, application of the most efficient of them for the geodynamo task is regardered.
A.S. Chemarev +2 more
doaj +1 more source
On the Precession Driven Geodynamo [PDF]
Formation of flow structures in the Earth’s liquid core enclosed in a precessing and rotating shell (mantle) is examined within the hydrodynamic approach. The kinematics and energetics of the motions in the Earth’s core initiated by precession allow one to regard these motions as a possible geodynamo mechanism at an early evolutionary stage of the ...
openaire +1 more source
Probabilistic structure of the geodynamo
One of the most intriguing features of Earth's axial magnetic dipole field, well-known from the geological record, is its occasional and unpredictable reversal of polarity. Understanding the phenomenon is rendered very difficult by the highly non-linear nature of the underlying magnetohydrodynamic problem. Numerical simulations of the liquid outer core,
Scullard, Christian R, Buffett, Bruce A
openaire +5 more sources
The geodynamo for non-geophysicists
The geodynamo usually appears as a somewhat intimidating subject. Its understanding seems to require knowledge of the intricate theory of magnetohydrodynamics. The solution of the corresponding equations can only be achieved numerically. It seems to be a
Herrmann, Friedrich, Vorbach, Tobias
core +1 more source
The Cretaceous Normal Superchron (CNS) was first defined in the 1960s to explain the Cretaceous Quiet Zone in marine magnetic anomaly profiles, which includes no or fewer geomagnetic reversals.
Yutaka Yoshimura
doaj +1 more source
Stochastic Models of Geodynamo Simulations [PDF]
The Earth's magnetic field originates primarily in the interior of the planet, and represents one of the few signals through which processes of the deep Earth are expressed at the surface.
Davis, William
core
Asymmetric Dipole Trends in Geodynamo Models and the Paleomagnetic Field
Temporal trends in the paleomagnetic dipole moment exhibit the property of positive skewness. On average, positive trends are larger and occur less frequently than negative trends over timescales of several tens of kyr.
B. A. Buffett
doaj +1 more source
The influence of potassium on core and geodynamo evolution [PDF]
We model the thermal evolution of the core and mantle using a parametrized convection scheme, and calculate the entropy available to drive the geodynamo as a function of time.
Brodholt, J. +3 more
core +1 more source
Paleomagnetic Biases Inferred From Numerical Dynamos and the Search for Geodynamo Evolution
The paleomagnetic record is central to our understanding of the history of the Earth. The orientation and intensity of magnetic minerals preserved in ancient rocks indicate the geodynamo has been alive since at least the Archean and possibly the Hadean ...
Peter E. Driscoll, Cian Wilson
doaj +1 more source

