Turbulence in anisotropic heliospheric plasmas

Details Turbulence in anisotropic heliospheric plasmas Turbulence in anisotropic heliospheric plasmas

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008sf2a.conf..547b&link_type=abstract

"SF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: C. Charbonnel, F. Combes

Astronomy and Astrophysics

Astrophysics

Scientific paper

An alternative approach to Direct Numerical Simulations (DNS) of Magnetohydrodynamics (MHD) is presented, providing insight into the statistical properties of highly-turbulent, intermittent, anisotropic MHD turbulence: a set of shell-models coupled by Alfvén waves travelling along the axial magnetic field and which interact non-linearly, producing perpendicular fluctuations of the fields at small scales. This model can be applied to different physical situations; we present the cases of heating in solar coronal loops, and of turbulence in open coronal regions at the base of the solar wind.

Affiliated with

Also associated with

No associations

Rating

Turbulence in anisotropic heliospheric plasmas does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Turbulence in anisotropic heliospheric plasmas, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Turbulence in anisotropic heliospheric plasmas will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1287911