TY - GEN
T1 - A Lagrangian Method for Extracting Eddy Boundaries in the Red Sea and the Gulf of Aden
AU - Friederici, Anke
AU - Toye, Habib
AU - Hoteit, Ibrahim
AU - Weinkauf, Tino
AU - Theisel, Holger
AU - Hadwiger, Markus
N1 - KAUST Repository Item: Exported on 2020-10-01
Acknowledgements: This work was supported in part by funding from King Abdullah University of Science and Technology (KAUST).
PY - 2019/9/5
Y1 - 2019/9/5
N2 - Mesoscale ocean eddies play a major role for both the intermixing of water and the transport of biological mass. This makes the identification and tracking of their shape, location and deformation over time highly important for a number of applications. While eddies maintain a roughly circular shape in the free ocean, the narrow basins of the Red Sea and Gulf of Aden lead to the formation of irregular eddy shapes that existing methods struggle to identify. We propose the following model: Inside an eddy, particles rotate around a common core and thereby remain at a constant distance under a certain parametrization. The transition to the more unpredictable flow on the outside can thus be identified as the eddy boundary. We apply this algorithm on a realistic simulation of the Red Sea circulation, where we are able to identify the shape of irregular eddies robustly and more coherently than previous methods. We visualize the eddies as tubes in space-time to enable the analysis of their movement and deformation over several weeks.
AB - Mesoscale ocean eddies play a major role for both the intermixing of water and the transport of biological mass. This makes the identification and tracking of their shape, location and deformation over time highly important for a number of applications. While eddies maintain a roughly circular shape in the free ocean, the narrow basins of the Red Sea and Gulf of Aden lead to the formation of irregular eddy shapes that existing methods struggle to identify. We propose the following model: Inside an eddy, particles rotate around a common core and thereby remain at a constant distance under a certain parametrization. The transition to the more unpredictable flow on the outside can thus be identified as the eddy boundary. We apply this algorithm on a realistic simulation of the Red Sea circulation, where we are able to identify the shape of irregular eddies robustly and more coherently than previous methods. We visualize the eddies as tubes in space-time to enable the analysis of their movement and deformation over several weeks.
UR - http://hdl.handle.net/10754/656836
UR - https://ieeexplore.ieee.org/document/8823600/
UR - http://www.scopus.com/inward/record.url?scp=85072950209&partnerID=8YFLogxK
U2 - 10.1109/scivis.2018.8823600
DO - 10.1109/scivis.2018.8823600
M3 - Conference contribution
SN - 9781538668825
SP - 52
EP - 56
BT - 2018 IEEE Scientific Visualization Conference (SciVis)
PB - IEEE
ER -