4.7 Article

ALFVENIC TURBULENCE BEYOND THE AMBIPOLAR DIFFUSION SCALE

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

  1. NASA Einstein Fellowship
  2. Center for Magnetic Self-Organization in Astrophysical and Laboratory Plasmas
  3. Physics Graduate Program/UFRN, at Natal
  4. NSF [AST 1212096, NSF-AST-1009091, NSF-ACI-1307369, NSF-DMS-1361197]
  5. NASA grants from the Fermi program
  6. NASA-NNX [12A088G]
  7. National R AMP
  8. D Program through the National Research Foundation of Korea (NRF) - Ministry of Education [2011-0012081]
  9. National Research Foundation of Korea [2011-0012081] Funding Source: Korea Institute of Science & Technology Information (KISTI), National Science & Technology Information Service (NTIS)
  10. Direct For Computer & Info Scie & Enginr
  11. Office of Advanced Cyberinfrastructure (OAC) [1307369] Funding Source: National Science Foundation
  12. Direct For Mathematical & Physical Scien
  13. Division Of Astronomical Sciences [1212096] Funding Source: National Science Foundation
  14. Direct For Mathematical & Physical Scien
  15. Division Of Mathematical Sciences [1361197] Funding Source: National Science Foundation
  16. Direct For Mathematical & Physical Scien
  17. Division Of Physics [821899] Funding Source: National Science Foundation
  18. Division Of Astronomical Sciences
  19. Direct For Mathematical & Physical Scien [GRANTS:13775080] Funding Source: National Science Foundation

向作者/读者索取更多资源

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.).

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.7
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据