Stochasticity and Complexity in Space Plasmas and the Dynamic Renormalization Group

Details Stochasticity and Complexity in Space Plasmas and the Dynamic Renormalization Group Stochasticity and Complexity in Space Plasmas and the Dynamic Renormalization Group

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agusmsm42a..07c&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SM42A-07

Physics

Geophysics

4400 Nonlinear Geophysics (3200, 6944, 7839), 4420 Chaos (7805), 7863 Turbulence (4490)

Scientific paper

A modern description of dynamical stochasticity and complexity relevant to the intermittent turbulence of coexisting nonpropagating spatiotemporal fluctuations and propagating modes in space plasmas is provided. The theory is based on the physical concepts of sporadic and localized interactions of coherent structures that emerge naturally from plasma resonances. The technique of the dynamic renormalization group is applied to the study of forced and/or self-organized criticality (FSOC), scale invariance, and symmetry breaking, related to such type of multiscale fluctuations. Numerical examples are presented to illustrate the concepts and methodology.

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