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EVOLUTION OF DENSITY PERTURBATIONS IN A CYLINDRICAL MOLECULAR CLOUD USING SMOOTHED PARTICLE HYDRODYNAMICS
ISM: clouds evolution ISM: magnetic fields Stars: formation Methods: numerical
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2010/10/29
Molecular clouds have a hierarchical structure from few tens of
parsecs for giants to few tenth of a parsec for proto-stellar cores. Nowadays, our
observational techniques are so advanced that it ha...
Self-Advection of Density Perturbations on a Sloping Continental Shelf
Density Perturbations Self-Advection Sloping Continental Shelf
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2009/2/5
Bottom water movement on the continental shelf is modeled by the nonlinear interaction between long-shore bottom geostrophic flow and the density field. Bottom geostrophic velocity, subject to linear ...
Influence of the Solar and Density Perturbations on the Neutrino Parameters
the Solar and Density Perturbations the Neutrino Parameters
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2010/10/27
There are reasons to believe that the solar matter density fluctuates around an equilibrium profile. One of these reasons is a resonance between the Alfv´en waves and the g-modes inside the Sun ...