Published October 2018
| Supplemental Material + Accepted Version + Published
Journal Article
Open
Mandala-inspired representation of the turbulent energy cascade
Chicago
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Abstract
This paper is associated with a poster winner of a 2017 APS/DFD Milton van Dyke Award for work presented at the DFD Gallery of Fluid Motion. The original poster is available from the Gallery of Fluid Motion, https://doi.org/10.1103/APS.DFD.2017.GFM.P0026
Additional Information
© 2018 Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. Received 27 January 2018; published 17 October 2018. The authors are grateful to Prof. Yukio Kaneda and Prof. Takashi Ishihara for providing the data and thank Prof. Geoffrey Spedding and Mark Fischer for useful discussions. M.B. acknowledges support from the Advanced Simulation and Computing program of the US Department of Energy's National Nuclear Security Administration via the PSAAP-II Center at Stanford (Grant No. 107908). H.J.B. and A.L.-D. acknowledge the support of NASA Transformative Aeronautics Concepts Program (Grant No. UNIX15AU93A).Attached Files
Published - PhysRevFluids.3.100505.pdf
Accepted Version - nihms-1050996.pdf
Supplemental Material - GOFM_BassenneBaeLozanoDuran_large.png
Files
PhysRevFluids.3.100505.pdf
Additional details
- PMCID
- PMC6800704
- Eprint ID
- 108432
- Resolver ID
- CaltechAUTHORS:20210315-111745889
- Department of Energy (DOE)
- 107908
- NASA
- UNIX15AU93A
- Created
-
2021-03-19Created from EPrint's datestamp field
- Updated
-
2021-03-19Created from EPrint's last_modified field
- Caltech groups
- GALCIT