期刊
ASTROPHYSICAL JOURNAL
卷 805, 期 2, 页码 -出版社
IOP Publishing Ltd
DOI: 10.1088/0004-637X/805/2/118
关键词
magnetohydrodynamics (MHD); turbulence; waves
资金
- NASA Einstein Fellowship
- Center for Magnetic Self-Organization in Astrophysical and Laboratory Plasmas
- Physics Graduate Program/UFRN, at Natal
- NSF [AST 1212096, NSF-AST-1009091, NSF-ACI-1307369, NSF-DMS-1361197]
- NASA grants from the Fermi program
- NASA-NNX [12A088G]
- National R AMP
- D Program through the National Research Foundation of Korea (NRF) - Ministry of Education [2011-0012081]
- National Research Foundation of Korea [2011-0012081] Funding Source: Korea Institute of Science & Technology Information (KISTI), National Science & Technology Information Service (NTIS)
- Direct For Computer & Info Scie & Enginr
- Office of Advanced Cyberinfrastructure (OAC) [1307369] Funding Source: National Science Foundation
- Direct For Mathematical & Physical Scien
- Division Of Astronomical Sciences [1212096] Funding Source: National Science Foundation
- Direct For Mathematical & Physical Scien
- Division Of Mathematical Sciences [1361197] Funding Source: National Science Foundation
- Direct For Mathematical & Physical Scien
- Division Of Physics [821899] Funding Source: National Science Foundation
- Division Of Astronomical Sciences
- Direct For Mathematical & Physical Scien [GRANTS:13775080] Funding Source: National Science Foundation
We investigate the nature of the Alfvenic 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 (L-AD). Using mode decomposition to separate the three classical MHD modes, we study the second-order structure functions of the Alfven mode velocity field of both neutrals and ions in the reference frame of the local magnetic field. On scales greater than L-AD 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 L-AD. We find that Alfvenic turbulence can exist past L-AD when the turbulence is globally super-Alfvenic, with the ions and neutrals forming separate cascades once decoupling has taken place. When turbulence is globally sub-Alfvenic and hence strongly anisotropic, with a large separation between the parallel and perpendicular decoupling scales, turbulence is damped at L-AD. 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.).
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