the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Applying dynamical systems techniques to real ocean drifters
Abstract. This paper presents the first comprehensive comparison of several different dynamical-systems-based measures of stirring and Lagrangian coherence, computed from real ocean drifters. Seven commonly used methods (finite-time Lyapunov exponent, trajectory path length, trajectory correlation dimension, trajectory encounter volume, Lagrangian-averaged vorticity deviation, dilation, and spectral clustering) were applied to 135 surface drifters in the Gulf of Mexico in order to map out the dominant Lagrangian coherent structures. Among the detected structures were regions of hyperbolic nature resembling stable manifolds from classical examples, divergent and convergent zones, and groups of drifters that moved more coherently and stayed closer together than the rest of the drifters. Many methods highlighted the same structures, but there were differences too. Overall, 5 out of 7 methods provided useful information about the geometry of transport within the domain spanned by the drifters.
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Notice on discussion status
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
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Preprint
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Supplement
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The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(2059 KB) - Metadata XML
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Supplement
(3334 KB) - BibTeX
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- Final revised paper
Journal article(s) based on this preprint
Interactive discussion
Status: closed
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RC1: 'Comment on egusphere-2022-250', Anonymous Referee #1, 19 May 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-250/egusphere-2022-250-RC1-supplement.pdf
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AC1: 'Reply on RC1', Irina I. Rypina, 15 Aug 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-250/egusphere-2022-250-AC1-supplement.pdf
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AC1: 'Reply on RC1', Irina I. Rypina, 15 Aug 2022
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RC2: 'Comment on egusphere-2022-250', Anonymous Referee #2, 30 Jun 2022
Please find my review in the attached document.
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AC2: 'Reply on RC2', Irina I. Rypina, 15 Aug 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-250/egusphere-2022-250-AC2-supplement.pdf
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AC2: 'Reply on RC2', Irina I. Rypina, 15 Aug 2022
Interactive discussion
Status: closed
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RC1: 'Comment on egusphere-2022-250', Anonymous Referee #1, 19 May 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-250/egusphere-2022-250-RC1-supplement.pdf
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AC1: 'Reply on RC1', Irina I. Rypina, 15 Aug 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-250/egusphere-2022-250-AC1-supplement.pdf
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AC1: 'Reply on RC1', Irina I. Rypina, 15 Aug 2022
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RC2: 'Comment on egusphere-2022-250', Anonymous Referee #2, 30 Jun 2022
Please find my review in the attached document.
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AC2: 'Reply on RC2', Irina I. Rypina, 15 Aug 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-250/egusphere-2022-250-AC2-supplement.pdf
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AC2: 'Reply on RC2', Irina I. Rypina, 15 Aug 2022
Peer review completion
Journal article(s) based on this preprint
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Cited
1 citations as recorded by crossref.
Timothy Getscher
Lawrence Pratt
Tamay Ozgokmen
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(2059 KB) - Metadata XML
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Supplement
(3334 KB) - BibTeX
- EndNote
- Final revised paper