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AGU: Journal of Geophysical Research, Space Physics

 

Keywords

  • Alfvén waves
  • solar-terrestrial environment
  • space plasmas
  • solar wind
  • chaos
  • intermittency

Index Terms

  • Interplanetary Physics: Solar wind plasma
  • Interplanetary Physics: MHD waves and turbulence
  • Nonlinear Geophysics: Bifurcations and attractors
  • Nonlinear Geophysics: Chaos
  • Computational Geophysics: Numerical solutions
Abstract
Cited By (4)
 

Abstract

JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 111, A07S03, 16 PP., 2006
doi:10.1029/2005JA011396

On the chaotic nature of solar-terrestrial environment: Interplanetary Alfvén intermittency

A. C.-L. Chian

National Institute for Space Research (INPE) and World Institute for Space Environment Research (WISER), São José dos Campos, São Paulo, Brazil

Nagoya University, Solar-Terrestrial Environment Laboratory, Toyokawa, Japan

Y. Kamide

Nagoya University, Solar-Terrestrial Environment Laboratory, Toyokawa, Japan

E. L. Rempel

Institute of Aeronautical Technology (ITA) and World Institute for Space Environment Research (WISER), São José dos Campos, São Paulo, Brazil

W. M. Santana

National Institute for Space Research (INPE) and World Institute for Space Environment Research (WISER), São José dos Campos, São Paulo, Brazil

We present an overview of observational and theoretical evidence of chaos and intermittency in the solar-terrestrial environment including solar dynamo, solar atmosphere, solar wind, and terrestrial magnetosphere-ionosphere-atmosphere. The chaotic nature of space plasmas is studied by a nonlinear model of Alfvén waves described by the low-dimensional limit of the derivative nonlinear Schrödinger equation given by its stationary solutions in the frame moving with the driver wave velocity. A periodic window of the bifurcation diagram is constructed to identify two types of Alfvén chaos related to type-I intermittency and crisis-induced intermittency. We show that an Alfvén chaotic attractor is composed of chaotic saddles and unstable periodic orbits and explain the links between these unstable structures and Alfvén intermittency. The role of interplanetary Alfvén intermittency in the solar wind driving of intense geomagnetic activities is discussed.

Received 31 August 2005; accepted 3 May 2006; published 7 July 2006.

Citation: Chian, A. C.-L., Y. Kamide, E. L. Rempel, and W. M. Santana (2006), On the chaotic nature of solar-terrestrial environment: Interplanetary Alfvén intermittency, J. Geophys. Res., 111, A07S03, doi:10.1029/2005JA011396.

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