scholarly journals The role of viscoelastic foundation on flexural gravity wave blocking in shallow water

AIP Advances ◽  
2021 ◽  
Vol 11 (6) ◽  
pp. 065317
Author(s):  
S. Boral ◽  
S. Nath ◽  
T. Sahoo ◽  
Michael H. Meylan
Keyword(s):  
Shallow Water ◽  
Gravity Wave ◽  
Viscoelastic Foundation ◽  
Wave Blocking ◽  
Flexural Gravity Wave

Flexural-gravity wave motion in the presence of shear current: Wave blocking and negative energy waves

2018 ◽  
Vol 30 (10) ◽  
pp. 106606 ◽  
Author(s):  
Santu Das ◽  
Prakash Kar ◽  
Trilochan Sahoo ◽  
Michael H. Meylan
Keyword(s):  
Gravity Wave ◽  
Wave Motion ◽  
Negative Energy ◽  
Current Wave ◽  
Shear Current ◽  
Wave Blocking ◽  
Flexural Gravity Wave

scholarly journals Numerical Simulations of a Gravity Wave Event over CCOPE. Part I: The Role of Geostrophic Adjustment in Mesoscale Jetlet Formation

1997 ◽  
Vol 125 (6) ◽  
pp. 1185-1211 ◽  
Author(s):  
Michael L. Kaplan ◽  
Steven E. Koch ◽  
Yuh-Lang Lin ◽  
Ronald P. Weglarz ◽  
Robert A. Rozumalski
Keyword(s):  
Numerical Simulations ◽  
Gravity Wave ◽  
Geostrophic Adjustment ◽  
Wave Event

Role of gravity wave seed perturbations in ESF day-to-day variability: A quantitative approach

2016 ◽  
Vol 57 (4) ◽  
pp. 1021-1028 ◽  
Author(s):  
G. Manju ◽  
M.K. Madhav Haridas ◽  
R.P. Aswathy
Keyword(s):  
Gravity Wave ◽  
Quantitative Approach

scholarly journals A shallow water analogue of asymmetric core-collapse, and neutron star kick/spin

2011 ◽  
Vol 7 (S279) ◽  
pp. 134-137
Author(s):  
Thierry Foglizzo ◽  
Frédéric Masset ◽  
Jérôme Guilet ◽  
Gilles Durand
Keyword(s):  
Neutron Star ◽  
Shallow Water ◽  
Acoustic Waves ◽  
Large Scale ◽  
Massive Stars ◽  
Core Collapse ◽  
Hydraulic Jumps ◽  
Core Collapse Supernova ◽  
Accretion Shock

AbstractMassive stars end their life with the gravitational collapse of their core and the formation of a neutron star. Their explosion as a supernova depends on the revival of a spherical accretion shock, located in the inner 200km and stalled during a few hundred milliseconds. Numerical simulations suggest that the large scale asymmetry of the neutrino-driven explosion is induced by a hydrodynamical instability named SASI. Its non radial character is able to influence the kick and the spin of the resulting neutron star. The SWASI experiment is a simple shallow water analog of SASI, where the role of acoustic waves and shocks is played by surface waves and hydraulic jumps. Distances in the experiment are scaled down by a factor one million, and time is slower by a factor one hundred. This experiment is designed to illustrate the asymmetric nature of core-collapse supernova.

Standing Gravity Wave Regimes in a Shallow-Water Resonator

2018 ◽  
pp. 63-75
Author(s):  
Alexey Slunyaev ◽  
Alexander Ezersky ◽  
Dominique Mouaze ◽  
Wuttersack Chokchai
Keyword(s):  
Shallow Water ◽  
Gravity Wave
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