MHD turbulence model for global simulations of the solar wind and SEP acceleration

Details MHD turbulence model for global simulations of the solar wind and SEP acceleration MHD turbulence model for global simulations of the solar wind and SEP acceleration

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1039...93s&link_type=abstract

PARTICLE ACCELERATION AND TRANSPORT IN THE HELIOSPHERE AND BEYOND: 7th Annual International Astrophysics Conference. AIP Confer

Astronomy and Astrophysics

Astrophysics

Magnetohydrodynamics And Plasmas, Turbulence, Flares, Planetary Bow Shocks, Interplanetary Shocks, Plasma Temperature And Density, X- And Gamma-Ray Telescopes And Instrumentation, Magnetohydrodynamic Waves

Scientific paper

The aim of the present work is to unify the various transport equations
for turbulent waves that are used in different areas of space physics.
We mostly focus on the magnetohydrodynamic (MHD) turbulence, in
particular the Alfvénic turbulence.

Affiliated with

Also associated with

No associations

Rating

MHD turbulence model for global simulations of the solar wind and SEP acceleration 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 MHD turbulence model for global simulations of the solar wind and SEP acceleration, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and MHD turbulence model for global simulations of the solar wind and SEP acceleration will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1170964