Alfvén Intermittent Turbulence Driven by Temporal Chaos

Details Alfvén Intermittent Turbulence Driven by Temporal Chaos Alfvén Intermittent Turbulence Driven by Temporal Chaos

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998apj...505..993c&link_type=abstract

The Astrophysical Journal, Volume 505, Issue 2, pp. 993-998.

Astronomy and Astrophysics

Astronomy

17

Chaos, Magnetohydrodynamics: Mhd, Plasmas, Sun: Solar Wind, Turbulence

Scientific paper

The temporal evolution of Alfvén intermittent turbulence in cosmic plasmas is studied. The chaotic dynamics of a driven-dissipative Alfvén system is determined by numerically solving the derivative nonlinear Schrödinger equation in the low-dimensional limit. Two types of Alfvén intermittent turbulence are identified: Pomeau-Manneville intermittency and crisis-induced intermittency. The significance of this theory for Alfvénic intermittent turbulence observed in the solar wind is discussed.

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