Scale-dependent anistropy in gyrokinetic turbulence

Details Scale-dependent anistropy in gyrokinetic turbulence Scale-dependent anistropy in gyrokinetic turbulence

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aps..apr.k1003k&link_type=abstract

American Physical Society, APS April Meeting 2012, March 31-Apr 3, 2012, abstract #K1.003

Astronomy and Astrophysics

Astronomy

Scientific paper

Eddies in Alfvenic turbulence get progressively more anisotropic with respect to the local magnetic field. This has been recently observed in a gyrokinetic simulation [Howes et. al., PRL, 107:035004:2011, TenBarge & Howes, eprint arXiv:1201.0056]. However, the nature of cascade for slow modes in an Alfvenic turbulent bath is still unclear. We present theory and numerical results from AstroGK exploring the nature of this cascade.

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