Magnetohydrodynamics in rapidly rotating spherical systems

K Zhang, G Schubert - Annual review of fluid mechanics, 2000 - annualreviews.org
▪ Abstract Recent developments in the study of buoyancy-driven convection,
magnetoconvection, and convection-driven dynamos in rapidly rotating spherical systems …

[图书][B] Physics of the Earth

FD Stacey, PM Davis - 2008 - books.google.com
The fourth edition of Physics of the Earth maintains the original philosophy of this classic
graduate textbook on fundamental solid earth geophysics, while being completely revised …

A three-dimensional convective dynamo solution with rotating and finitely conducting inner core and mantle

GA Glatzmaier, PH Roberts - Physics of the Earth and Planetary Interiors, 1995 - Elsevier
We present the first three-dimensional (3D), time-dependent, self-consistent numerical
solution of the magneto-hydrodynamic (MHD) equations that describe thermal convection …

The distinction between geomagnetic excursions and reversals

D Gubbins - Geophysical Journal International, 1999 - academic.oup.com
Two recent studies of the geomagnetic field in the last 1Myr have found 14 excursions, large
changes in direction lasting 5–10kyr each, six of which are established as global …

The magnetic field of planet Earth

G Hulot, CC Finlay, CG Constable, N Olsen… - Planetary …, 2010 - Springer
The magnetic field of the Earth is by far the best documented magnetic field of all known
planets. Considerable progress has been made in our understanding of its characteristics …

[图书][B] Mathematical aspects of natural dynamos

E Dormy, AM Soward - 2007 - taylorfrancis.com
Although the origin of Earth's and other celestial bodies' magnetic fields remains unknown,
we do know that the motion of electrically conducting fluids generates and maintains these …

The deep interior of Venus, Mars, and the Earth: A brief review and the need for planetary surface-based measurements

A Mocquet, P Rosenblatt, V Dehant… - Planetary and Space …, 2011 - Elsevier
A comparison of the internal structure of Earth-like planets is unavoidable to understand the
formation and evolution of the solar system, and the differences between Earth's, Mars', and …

Numerical dynamo models of Uranus' and Neptune's magnetic fields

S Stanley, J Bloxham - Icarus, 2006 - Elsevier
The non-axisymmetric, non-dipolar magnetic fields of Uranus and Neptune are markedly
different from the axially-dipolar dominated fields of the other planets in our Solar System …

Rapid changes of magnetic Field polarity in the late Ediacaran: Linking the Cambrian evolutionary radiation and increased UV-B radiation

JG Meert, NM Levashova, ML Bazhenov, E Landing - Gondwana Research, 2016 - Elsevier
Novelty in the biological world is the culmination of genetic changes often triggered by the
physical environment. The most radical phase of biological evolution took place during the …

[HTML][HTML] Shallow bias of paleomagnetic inclinations in the Paleozoic and Precambrian

DV Kent, MA Smethurst - Earth and Planetary Science Letters, 1998 - Elsevier
An updated analysis of the global paleomagnetic database shows that the frequency
distributions of paleomagnetic inclinations for the Cenozoic and Mesozoic eras (younger …