FN Archimer Export Format
PT J
TI Optimal Perturbations of an Oceanic Vortex Lens
BT
AF MEUNIER, Thomas
MENESGUEN, Claire
CARTON, Xavier
LE GENTIL, Sylvie
SCHOPP, Richard
AS 1:1;2:2;3:3;4:2;5:4;
FF 1:;2:PDG-ODE-LOPS-OH;3:;4:PDG-ODE-LOPS-OH;5:;
C1 Ctr Invest Cient & Educ Super Ensenada, Dept Oceanog Fis, Ensenada 22860, Baja California, Mexico.
IFREMER, Lab Oceanog Phys & Spatiale, F-29280 Plouzane, France.
Inst Univ Europeen Mer, Lab Oceanog Phys & Spatiale, F-29280 Plouzane, France.
C2 CICESE, MEXICO
IFREMER, FRANCE
UBO, FRANCE
CNRS, FRANCE
SI BREST
SE PDG-ODE-LOPS-OH
UM LOPS
IN WOS Ifremer jusqu'en 2018
DOAJ
copubli-france
copubli-univ-france
copubli-int-hors-europe
copubli-sud
TC 3
UR https://archimer.ifremer.fr/doc/00454/56605/58297.pdf
LA English
DT Article
DE ;vortex lenses;intrathermocline eddies;instability;optimal perturbations
AB The stability properties of a vortex lens are studied in the quasi geostrophic (QG) framework using the generalized stability theory. Optimal perturbations are obtained using a tangent linear QG model and its adjoint. Their fine-scale spatial structures are studied in details. Growth rates of optimal perturbations are shown to be extremely sensitive to the time interval of optimization: The most unstable perturbations are found for time intervals of about 3 days, while the growth rates continuously decrease towards the most unstable normal mode, which is reached after about 170 days. The horizontal structure of the optimal perturbations consists of an intense counter-shear spiralling. It is also extremely sensitive to time interval: for short time intervals, the optimal perturbations are made of a broad spectrum of high azimuthal wave numbers. As the time interval increases, only low azimuthal wave numbers are found. The vertical structures of optimal perturbations exhibit strong layering associated with high vertical wave numbers whatever the time interval. However, the latter parameter plays an important role in the width of the vertical spectrum of the perturbation: short time interval perturbations have a narrow vertical spectrum while long time interval perturbations show a broad range of vertical scales. Optimal perturbations were set as initial perturbations of the vortex lens in a fully non linear QG model. It appears that for short time intervals, the perturbations decay after an initial transient growth, while for longer time intervals, the optimal perturbation keeps on growing, quickly leading to a non-linear regime or exciting lower azimuthal modes, consistent with normal mode instability. Very long time intervals simply behave like the most unstable normal mode. The possible impact of optimal perturbations on layering is also discussed
PY 2018
PD SEP
SO Fluids
SN 2311-5521
PU Mdpi
VL 3
IS 3
UT 000447921200019
DI 10.3390/fluids3030063
ID 56605
ER
EF