Published August 10, 2015 | Version v1
Journal article

On the emergence of a 1/k spectrum in the sub-inertial domain of turbulent media

  • 1. INAF-Istituto di Astrofisica e Planetologia Spaziali, Roma (Italy)
  • 2. Dip. di Fisica, Università della Calabria, Rende (CS) (Italy)

Description

Several physical and astrophysical fluid and plasma systems displaying turbulent features show a 1/k (or 1/f) spectral domain at spatial (temporal) scales above the inertial range. Here, we investigate the formation of a 1/k spectral domain in fluid and MHD turbulence systems in the sub-inertial range ( k < k 0 , where k0 is the injection scale) by means of shell-model simulations. The simulation results suggest that the 1/k domain emerges as a consequence of competing direct and inverse cascading processes, implying the formation and dissipation of large-scale gradients below the inertial domain. The relevance of our results for observations in space and astrophysical contexts is briefly discussed.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-637X/809/1/21

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
809
Journal Issue
1
Series
Since 2009, the country of publication for this journal is the UK.
Journal Page Range
[6 p.]
ISSN
0004-637X
CODEN
ASJOAB

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
51045101
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ASTROPHYSICS; COMPUTERIZED SIMULATION; MAGNETOHYDRODYNAMICS; PLASMA; SHELL MODELS; SPACE; SPECTRA; TURBULENCE
Descriptors DEC
FLUID MECHANICS; HYDRODYNAMICS; MATHEMATICAL MODELS; MECHANICS; NUCLEAR MODELS; PHYSICS; SIMULATION