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Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have found the clearest evidence yet that giant planets have recently formed around four young stars. These new worlds, each p...
We present a dynamo mechanism arising from the presence of barotropically unstable zonal jet currents in a spherical shell. The shear instability of the zonal flow develops in the form of a global Ros...
Three dimensional studies of convection in deep spherical shells have been used to test the hypothesis that the strong jet streams on Jupiter, Saturn, Uranus, and Neptune result from convection throug...
Magnetospheric accretion is an important process for a wide range of astrophysical systems, and may play a role in the formation of gas giant planets. Extending the formalism describing stellar magnet...
Evolution of Gas Giant Planets Using the Core Accretion Model     Planets  Core Accretion Model       font style='font-size:12px;'> 2009/6/16
Evolution of Gas Giant Planets Using the Core Accretion Model。
Studies of Atmospheric Phenomena in the Giant Planets with Grantecan

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