Published June 1, 2015 | Version v1
Journal article

Alfvénic turbulence beyond the ambipolar diffusion scale

  • 1. Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 0213 (United States)
  • 2. Astronomy Department, University of Wisconsin, Madison, 475 N. Charter St., WI 53711 (United States)
  • 3. Department of Physics, University of Notre Dame, Notre Dame, IN 46556 (United States)
  • 4. Department of Astronomy and Space Science, Chungnam National University, Daejeon (Korea, Republic of)

Description

We investigate the nature of the Alfvénic turbulence cascade in two-fluid magnetohydrodynamic (MHD) simulations in order to determine if turbulence is damped once the ion and neutral species become decoupled at a critical scale called the ambipolar diffusion scale (LAD). Using mode decomposition to separate the three classical MHD modes, we study the second-order structure functions of the Alfvén mode velocity field of both neutrals and ions in the reference frame of the local magnetic field. On scales greater than LAD we confirm that two-fluid turbulence strongly resembles single-fluid MHD turbulence. Our simulations show that the behavior of two-fluid turbulence becomes more complex on scales less than LAD. We find that Alfvénic turbulence can exist past LAD when the turbulence is globally super-Alfvénic, with the ions and neutrals forming separate cascades once decoupling has taken place. When turbulence is globally sub-Alfvénic and hence strongly anisotropic, with a large separation between the parallel and perpendicular decoupling scales, turbulence is damped at LAD. We also find that the power spectrum of the kinetic energy in the damped regime is consistent with a k 4 scaling (in agreement with the predictions of Lazarian et al.).

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-637X/805/2/118

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
805
Journal Issue
2
Series
Since 2009, the country of publication for this journal is the UK.
Journal Page Range
[8 p.]
ISSN
0004-637X
CODEN
ASJOAB

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
51045392
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ALFVEN WAVES; AMBIPOLAR DIFFUSION; ANISOTROPY; COMPUTERIZED SIMULATION; DECOUPLING; FORECASTING; MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; SPECTRA; STRUCTURE FUNCTIONS; TURBULENCE; VELOCITY
Descriptors DEC
DIFFUSION; FLUID MECHANICS; FUNCTIONS; HYDRODYNAMICS; HYDROMAGNETIC WAVES; MECHANICS; SIMULATION