Far-dissipation range of turbulence.

نویسندگان

  • Chen
  • Doolen
  • Herring
  • Kraichnan
  • Orszag
  • She
چکیده

The very small scales of isotropic, Navier-Stokes turbulence at Reynolds number Rλ ≈ 15 are studied by high-resolution direct numerical simulation (DNS) and by integration of the direct-interaction (DIA) equations. The DNS follows the tail of the energy spectrum over more than thirty decades of magnitude. The energy spectrum in the far-dissipation range 5kd < k < 10kd is well-fitted by k α exp(−ck/kd), where kd is the Kolmogorov dissipation wavenumber, α ≈ 3.3 and c ≈ 7.1. For values of m that emphasize the fardissipation range, the fields (−∇2)mu exhibit strong spatial intermittency, associated with gentle spatial variations of the lower-k part of the velocity field. DIA analysis gives a prefactor k and an exponential decay more rapid than DNS. Averaging over an ensemble of DIA solutions, suggested by the observed intermittency, removes some of the discrepancy.

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

The Dissipation Range in Rotating Turbulence

The dissipation range energy balance of the direct interaction approximation is applied to rotating turbulence when rotation effects persist well into the dissipation range. Assuming that RoRe << 1 and that three-wave interactions are dominant, the dissipation range is found to be concentrated in the wavevector plane perpendicular to the rotation axis. This conclusion is consistent with previou...

متن کامل

Energy Spectrum in the Dissipation Range of Fluid Turbulence

High resolution, direct numerical simulations of three-dimensional incompressible Navier-Stokes equations are carried out to study the energy spectrum in the dissipation range. An energy spectrum of the form A(k/kd) _ exp[-/3k/kd] is confirmed. The possible values of the parameters c_ and/3, as well as their dependence on Reynolds numbers and length scales, are investigated, showing good agreem...

متن کامل

Thermodynamic structure of collision-dominated expanding plasma: Heating of interplanetary coronal mass ejections

[1] We investigate the thermodynamic structure of interplanetary coronal mass ejections (ICMEs) using combined surveys of the ejecta between 0.3 and 20 AU. ICMEs are shown to have a moderate expansion in the solar wind compared with theoretical predictions. The expansion seems to be governed by a polytrope with g 1.3 in this distance range. We find that Coulomb collisions are important contribu...

متن کامل

Multiscale Nature of the Dissipation Range in Gyrokinetic Simulations of Alfvénic Turbulence.

Nonlinear energy transfer and dissipation in Alfvén wave turbulence are analyzed in the first gyrokinetic simulation spanning all scales from the tail of the MHD range to the electron gyroradius scale. For typical solar wind parameters at 1 AU, about 30% of the nonlinear energy transfer close to the electron gyroradius scale is mediated by modes in the tail of the MHD cascade. Collisional dissi...

متن کامل

On the Rapid Increase of Intermittency in the Near-Dissipation Range of Fully Developed Turbulence

Intermittency, measured as log (F (r)/3), where F (r) is the flatness of velocity increments at scale r, is found to rapidly increase as viscous effects intensify, and eventually saturate at very small scales. This feature defines a finite intermediate range of scales between the inertial and dissipation ranges, that we shall call near-dissipation range. It is argued that intermittency is multi...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

عنوان ژورنال:
  • Physical review letters

دوره 70 20  شماره 

صفحات  -

تاریخ انتشار 1993