Published June 1, 2010 | Version v1
Journal article

NONLINEAR SIMULATION OF TURBULENT FIELD LINES AND COMPARISON OF THEIR MEAN CROSS-FIELD DISPLACEMENT WITH THEORETICAL PREDICTION

Creators

  • 1. Air Force Research Laboratory, RVBXS, 29 Randolph Rd., Hanscom AFB, MA 01731-3010 (United States)

Description

A new method for the full nonlinear computation of turbulent field lines is presented that extends the Sums of Random Numbers Distribution method previously applied to the computation of generalized quasilinear (GQL) field lines. A study of the mean cross-field displacement confirms the theoretical prediction of a nonlinear diffusion regime, on the large scales where the mean cross-field displacement exceeds twice the perpendicular correlation length. The simulation results duplicate at all length scales the variations of the mean cross-field displacement predicted by the theoretical calculations, including the transitions from GQL supradiffusion to nonlinear diffusion. Both GQL and full nonlinear computations also reproduce, accurately, the predicted variations with turbulence level of the large-scale GQL and nonlinear diffusion coefficients, respectively.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-637X/715/2/959

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
715
Journal Issue
2
Journal Page Range
p. 959-966
ISSN
0004-637X
CODEN
ASJOAB

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
42045835
Subject category
S97: MATHEMATICAL METHODS AND COMPUTING;
Descriptors DEI
CALCULATION METHODS; COMPUTERIZED SIMULATION; COSMIC RADIATION; MAGNETIC FIELDS; TURBULENCE
Descriptors DEC
IONIZING RADIATIONS; RADIATIONS; SIMULATION