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

Journal Article · Mon Aug 25 00:00:00 EDT 2008 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.2982491· OSTI ID:21152418

Sokolov, Igor V ^[1]; Roussev, Ilia I ^[2]

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1. Department of AOSS, University of Michigan, 2455 Hayward St, Ann Arbor, MI 48109 (United States)
2. Institute for Astronomy, University of Hawaii, 2680 Woodlawn Dr, Honolulu, HI 96822 (United States)

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 Alfvenic turbulence.

• OSTI ID: 21152418
• Journal Information: AIP Conference Proceedings, Vol. 1039, Issue 1; Conference: 7. annual international astrophysics conference, Kauai, HI (United States), 7-13 Mar 2008; Other Information: DOI: 10.1063/1.2982491; (c) 2008 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

70 PLASMA PHYSICS AND FUSION TECHNOLOGY
ACCELERATION
ALFVEN WAVES
COMPUTERIZED SIMULATION
MAGNETOHYDRODYNAMICS
PLASMA
PLASMA DENSITY
PLASMA SIMULATION
SHOCK WAVES
SOLAR FLARES
SOLAR WIND
TRANSPORT THEORY
TURBULENCE