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1997 (v1)PublicationUploaded on: March 27, 2023
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1998 (v1)Publication
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2017 (v1)Publication
Basic fluid equations are the main ingredient in the development of theories of Rayleigh-Taylor buoyancy-induced instability. Turbulence arises in the late stage of the instability evolution as a result of the proliferation of active scales of motion. Fluctuations are maintained by the unceasing conversion of potential energy into kinetic...
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1999 (v1)Publication
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Uploaded on: December 5, 2022 -
1997 (v1)Publication
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Uploaded on: December 5, 2022 -
1997 (v1)Publication
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1998 (v1)Publication
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1999 (v1)Publication
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1997 (v1)Publication
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2000 (v1)Publication
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2001 (v1)Publication
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2009 (v1)Publication
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2016 (v1)Publication
A state-of-the-art, in terms of spatio-temporal resolution (about 10 km and on a hourly basis) and temporal span (35 years), wave hindcast is exploited to update existing assessments of wave energy potential in the Mediterranean Sea. The hindcast, covering the period 1979–2013, has been obtained using WavewatchIII with calibrated source-term...
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1997 (v1)Publication
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2005 (v1)Publication
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2002 (v1)Publication
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2016 (v1)Publication
The turbulent Rayleigh-Taylor system in a rotating reference frame is investigated by direct numerical simulations within the Oberbeck-Boussinesq approximation. On the basis of theoretical arguments, supported by our simulations, we show that the Rossby number decreases in time, and therefore the Coriolis force becomes more important as the...
Uploaded on: March 27, 2023