---
_id: '662'
abstract:
- lang: eng
  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.'
article_number: '044107'
author:
- first_name: Liang
  full_name: Shi, Liang
  last_name: Shi
- first_name: Björn
  full_name: Hof, Björn
  id: 3A374330-F248-11E8-B48F-1D18A9856A87
  last_name: Hof
  orcid: 0000-0003-2057-2754
- first_name: Markus
  full_name: Rampp, Markus
  last_name: Rampp
- first_name: Marc
  full_name: Avila, Marc
  last_name: Avila
citation:
  ama: Shi L, Hof B, Rampp M, Avila M. Hydrodynamic turbulence in quasi Keplerian
    rotating flows. <i>Physics of Fluids</i>. 2017;29(4). doi:<a href="https://doi.org/10.1063/1.4981525">10.1063/1.4981525</a>
  apa: Shi, L., Hof, B., Rampp, M., &#38; Avila, M. (2017). Hydrodynamic turbulence
    in quasi Keplerian rotating flows. <i>Physics of Fluids</i>. American Institute
    of Physics. <a href="https://doi.org/10.1063/1.4981525">https://doi.org/10.1063/1.4981525</a>
  chicago: Shi, Liang, Björn Hof, Markus Rampp, and Marc Avila. “Hydrodynamic Turbulence
    in Quasi Keplerian Rotating Flows.” <i>Physics of Fluids</i>. American Institute
    of Physics, 2017. <a href="https://doi.org/10.1063/1.4981525">https://doi.org/10.1063/1.4981525</a>.
  ieee: L. Shi, B. Hof, M. Rampp, and M. Avila, “Hydrodynamic turbulence in quasi
    Keplerian rotating flows,” <i>Physics of Fluids</i>, vol. 29, no. 4. American
    Institute of Physics, 2017.
  ista: Shi L, Hof B, Rampp M, Avila M. 2017. Hydrodynamic turbulence in quasi Keplerian
    rotating flows. Physics of Fluids. 29(4), 044107.
  mla: Shi, Liang, et al. “Hydrodynamic Turbulence in Quasi Keplerian Rotating Flows.”
    <i>Physics of Fluids</i>, vol. 29, no. 4, 044107, American Institute of Physics,
    2017, doi:<a href="https://doi.org/10.1063/1.4981525">10.1063/1.4981525</a>.
  short: L. Shi, B. Hof, M. Rampp, M. Avila, Physics of Fluids 29 (2017).
date_created: 2018-12-11T11:47:47Z
date_published: 2017-04-01T00:00:00Z
date_updated: 2021-01-12T08:08:15Z
day: '01'
department:
- _id: BjHo
doi: 10.1063/1.4981525
intvolume: '        29'
issue: '4'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/1703.01714
month: '04'
oa: 1
oa_version: Submitted Version
project:
- _id: 2511D90C-B435-11E9-9278-68D0E5697425
  grant_number: SFB 963  TP A8
  name: Astrophysical instability of currents and turbulences
publication: Physics of Fluids
publication_identifier:
  issn:
  - '10706631'
publication_status: published
publisher: American Institute of Physics
publist_id: '7072'
quality_controlled: '1'
scopus_import: 1
status: public
title: Hydrodynamic turbulence in quasi Keplerian rotating flows
type: journal_article
user_id: 4435EBFC-F248-11E8-B48F-1D18A9856A87
volume: 29
year: '2017'
...