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 …
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 …
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 …
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 …
changes in direction lasting 5–10kyr each, six of which are established as global …
The magnetic field of planet Earth
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 …
planets. Considerable progress has been made in our understanding of its characteristics …
[图书][B] Mathematical aspects of natural dynamos
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 …
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 …
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
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 …
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 …
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 …
distributions of paleomagnetic inclinations for the Cenozoic and Mesozoic eras (younger …