Young, Roland M.B.Read, Peter L.Wang, Yixiong2025-07-302025-07-302019-07-01Young, R M B, Read, P L & Wang, Y 2019, 'Simulating Jupiter's weather layer. Part I : Jet spin-up in a dry atmosphere', Icarus, vol. 326, pp. 225-252. https://doi.org/10.1016/j.icarus.2018.12.0050019-1035ORCID: /0000-0002-7241-8954/work/154626157https://hdl.handle.net/2164/25781Funding Information: Support for RMBY and PLR provided by UK STFC Grants ST/F003145/1, ST/I001948/1, and ST/K00106X/1. Support for PLR provided by UK STFC Grant ST/N00082X/1. Part of this work was completed during a visit to the Kavli Institute for Theoretical Physics at UC Santa Barbara. This work was supported in part by the US National Science Foundation under Grant No. NSF PHY-1125915. The authors would like to thank Terry Davies, Nathan Mayne, William Ingram, Hiro Yamazaki, and Lena Zuchowski for assistance with an earlier version of the model, Pat Irwin and João Mendonça for help with the new radiation scheme, Liam Brannigan, Yuan Lian, David Munday and Inna Polichtchouk for assistance running the MITgcm, Jeremy Yates for his patience while we ran the simulations, Michael McIntyre, Aymeric Spiga, and Stephen Thomson for useful discussions, and two anonymous reviewers whose extensive comments improved the paper significantly. Many figures used David Fanning's Coyote IDL Program Library. This work used the DiRAC Data Centric system at Durham University, operated by the Institute for Computational Cosmology, and the Darwin Data Analytic system at the University of Cambridge, operated by the University of Cambridge HPC Service, both on behalf of the STFC DiRAC HPC Facility (www.dirac.ac.uk). This equipment was funded by BIS National E-infrastructure capital grants ST/K00042X/1 and ST/K001590/1, STFC capital grants ST/K00087X/1, ST/H008861/1, and ST/H00887X/1, DiRAC Operations grants ST/K003267/1 and ST/K00333X/1, and Durham University. DiRAC is part of the UK National E-Infrastructure. The authors acknowledge the use of the IRIDIS High Performance Computing Facility, and associated support services at the University of Southampton, in the completion of this work. The authors acknowledge the use of the University of Oxford Advanced Research Computing (ARC) facility in carrying out this work. http://dx.doi.org/10.5281/zenodo.22558.2812923592engBarotropic instabilityConvectionGeneral circulation modelJupiterSuper-rotationQB AstronomyAstronomy and AstrophysicsSpace and Planetary ScienceSTFC - Science and Technology Facilities CouncilST/F003145/1ST/I001948/1ST/K00106X/1ST/N00082X/1QBJournal article10.1016/j.icarus.2018.12.005http://www.scopus.com/inward/record.url?scp=85062210204&partnerID=8YFLogxK326