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 (, 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/809/1/21Additional 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