Jove
Visualize
Contact Us
JoVE
x logofacebook logolinkedin logoyoutube logo
ABOUT JoVE
OverviewLeadershipBlogJoVE Help Center
AUTHORS
Publishing ProcessEditorial BoardScope & PoliciesPeer ReviewFAQSubmit
LIBRARIANS
TestimonialsSubscriptionsAccessResourcesLibrary Advisory BoardFAQ
RESEARCH
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchive
EDUCATION
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualFaculty Resource CenterFaculty Site
Terms & Conditions of Use
Privacy Policy
Policies

Related Experiment Videos

Shell model for rotating turbulence.

Y Hattori1, R Rubinstein, A Ishizawa

  • 1Division of Computer Aided Science, Kyushu Institute of Technology, Tobata, Kitakyushu 804-8550, Japan.

Physical Review. E, Statistical, Nonlinear, and Soft Matter Physics
|December 17, 2004
PubMed
Summary
This summary is machine-generated.

Related Concept Videos

You might also read

Related Articles

Articles linked to this work by shared authors, journal, and citation graph.

Sort by
Same author

Turbulence Transition in Magnetically Confined Hydrogen and Deuterium Plasmas.

Physical review letters·2024
Same author

Characteristics of constrained turbulent transport in flux-driven toroidal plasmas.

Philosophical transactions. Series A, Mathematical, physical, and engineering sciences·2023
Same author

Measurement of Pa<sub>α</sub> line from pellet ablation cloud in Heliotron J.

The Review of scientific instruments·2022
Same author

Precise spectroscopy of <sup>167</sup>Er:Y<sub>2</sub>SiO<sub>5</sub> based on laser frequency stabilization using a fiber laser comb.

Optics express·2021
Same author

Persistence of Ion Temperature Gradient Turbulent Transport at Finite Normalized Pressure.

Physical review letters·2019
Same author

Application of portable near-infrared spectrometer to Heliotron J plasma diagnostics.

The Review of scientific instruments·2018
Same journal

Tension on dsDNA bound to ssDNA-RecA filaments may play an important role in driving efficient and accurate homology recognition and strand exchange.

Physical review. E, Statistical, nonlinear, and soft matter physics·2016
Same journal

Publisher's Note: Amplitude-phase coupling drives chimera states in globally coupled laser networks [Phys. Rev. E 91, 040901(R) (2015)].

Physical review. E, Statistical, nonlinear, and soft matter physics·2016
Same journal

Erratum: Shapes of sedimenting soft elastic capsules in a viscous fluid [Phys. Rev. E 92, 033003 (2015)].

Physical review. E, Statistical, nonlinear, and soft matter physics·2016
Same journal

Erratum: Attenuation of excitation decay rate due to collective effect [Phys. Rev. E 90, 022142 (2014)].

Physical review. E, Statistical, nonlinear, and soft matter physics·2016
Same journal

Publisher's Note: Role of connectivity and fluctuations in the nucleation of calcium waves in cardiac cells [Phys. Rev. E 92, 052715 (2015)].

Physical review. E, Statistical, nonlinear, and soft matter physics·2016
Same journal

Publisher's Note: Lattice Boltzmann approach for complex nonequilibrium flows [Phys. Rev. E 92, 043308 (2015)].

Physical review. E, Statistical, nonlinear, and soft matter physics·2016
See all related articles

This study introduces a modified shell model for rotating turbulence, finding that increased rotation changes the energy spectrum exponent. Numerical simulations and weak turbulence theory explain this phenomenon in fluid dynamics.

Area of Science:

  • * Physics
  • * Fluid Dynamics
  • * Turbulence

Background:

  • * Understanding the behavior of rotating turbulence is crucial in various fields, including astrophysics and geophysics.
  • * Existing models may not fully capture the complex effects of rotation on turbulent flows.
  • * The energy spectrum in turbulent flows describes how energy is distributed across different scales.

Purpose of the Study:

  • * To propose a modified shell model that incorporates the effects of rotation on turbulence.
  • * To investigate the impact of randomization in modeling rotational effects.
  • * To analyze the changes in the energy spectrum of rotating turbulence.

Main Methods:

  • * Development of a modified shell model including a randomized linear term to represent rotation.

Related Experiment Videos

  • * Conducting numerical simulations to observe the behavior of rotating turbulence.
  • * Applying weak turbulence theory to explain the observed spectral changes.
  • Main Results:

    • * The exponent of the energy spectrum in the inertial range shifts from -5/3 to -2 as the rotation rate increases.
    • * Randomization was found to be essential for accurately modeling the effect of rotation.
    • * Numerical results align with predictions from weak turbulence theory.

    Conclusions:

    • * The proposed modified shell model effectively captures the influence of rotation on turbulence.
    • * The observed spectral exponent change is a direct consequence of increased rotation.
    • * The study provides a theoretical and numerical framework for understanding rotating turbulence.