[{"date_updated":"2021-01-12T08:08:15Z","year":"2017","day":"01","department":[{"_id":"BjHo"}],"_id":"662","article_number":"044107","date_published":"2017-04-01T00:00:00Z","month":"04","citation":{"chicago":"Shi, Liang, Björn Hof, Markus Rampp, and Marc Avila. “Hydrodynamic Turbulence in Quasi Keplerian Rotating Flows.” Physics of Fluids. American Institute of Physics, 2017. https://doi.org/10.1063/1.4981525.","mla":"Shi, Liang, et al. “Hydrodynamic Turbulence in Quasi Keplerian Rotating Flows.” Physics of Fluids, vol. 29, no. 4, 044107, American Institute of Physics, 2017, doi:10.1063/1.4981525.","ista":"Shi L, Hof B, Rampp M, Avila M. 2017. Hydrodynamic turbulence in quasi Keplerian rotating flows. Physics of Fluids. 29(4), 044107.","ama":"Shi L, Hof B, Rampp M, Avila M. Hydrodynamic turbulence in quasi Keplerian rotating flows. Physics of Fluids. 2017;29(4). doi:10.1063/1.4981525","apa":"Shi, L., Hof, B., Rampp, M., & Avila, M. (2017). Hydrodynamic turbulence in quasi Keplerian rotating flows. Physics of Fluids. American Institute of Physics. https://doi.org/10.1063/1.4981525","short":"L. Shi, B. Hof, M. Rampp, M. Avila, Physics of Fluids 29 (2017).","ieee":"L. Shi, B. Hof, M. Rampp, and M. Avila, “Hydrodynamic turbulence in quasi Keplerian rotating flows,” Physics of Fluids, vol. 29, no. 4. American Institute of Physics, 2017."},"publication_status":"published","volume":29,"type":"journal_article","status":"public","intvolume":" 29","language":[{"iso":"eng"}],"publication_identifier":{"issn":["10706631"]},"publication":"Physics of Fluids","doi":"10.1063/1.4981525","author":[{"full_name":"Shi, Liang","first_name":"Liang","last_name":"Shi"},{"orcid":"0000-0003-2057-2754","full_name":"Hof, Björn","last_name":"Hof","first_name":"Björn","id":"3A374330-F248-11E8-B48F-1D18A9856A87"},{"last_name":"Rampp","first_name":"Markus","full_name":"Rampp, Markus"},{"full_name":"Avila, Marc","last_name":"Avila","first_name":"Marc"}],"publist_id":"7072","scopus_import":1,"project":[{"name":"Astrophysical instability of currents and turbulences","_id":"2511D90C-B435-11E9-9278-68D0E5697425","grant_number":"SFB 963 TP A8"}],"abstract":[{"text":"We report a direct-numerical-simulation study of the Taylor-Couette flow in the quasi-Keplerian regime at shear Reynolds numbers up to (105). Quasi-Keplerian rotating flow has been investigated for decades as a simplified model system to study the origin of turbulence in accretion disks that is not fully understood. The flow in this study is axially periodic and thus the experimental end-wall effects on the stability of the flow are avoided. Using optimal linear perturbations as initial conditions, our simulations find no sustained turbulence: the strong initial perturbations distort the velocity profile and trigger turbulence that eventually decays.","lang":"eng"}],"issue":"4","main_file_link":[{"url":"https://arxiv.org/abs/1703.01714","open_access":"1"}],"quality_controlled":"1","oa_version":"Submitted Version","title":"Hydrodynamic turbulence in quasi Keplerian rotating flows","user_id":"4435EBFC-F248-11E8-B48F-1D18A9856A87","publisher":"American Institute of Physics","oa":1,"date_created":"2018-12-11T11:47:47Z"}]