Author:
Prabin Devi S.,Singh S. B.,Surjalal Sharma A.
Abstract
Abstract. A test for deterministic dynamics in a time series data, namely the 0–1 test (Gottawald and Melbourne, 2004, 2005), is used to study the magnetospheric dynamics. The data, corresponding to the same time period, of the auroral electrojet index AL and the magnetic field component Bz of the solar wind magnetic field measured at 1 AU are used to compute the parameter K, which is zero for non-chaotic and unity for chaotic systems. For the magnetosphere and also for the turbulent solar wind, K has values corresponding to a nonlinear dynamical system with chaotic behaviour. This result is consistent with the Lyapunov exponents computed from the same time series data.
Reference46 articles.
1. Barrow, J. D. and Levin J.: A test of a test for chaos, arXiv:nlin/0303070v1, available at http://arxiv.org/abs/nlin0303070, 2003.
2. Bohr, T., Jensen, M. H., Paladin, G., and Vulpiani, A.: Dynamical Systems Approach to Turbulence, Cambridge University Press, Cambridge, UK, 1998.
3. Chang, T.: Self organized criticality, multifractal spectra, sporadic licalized reconnections and intermittent turbulence in the magnetotail, Phys. Plasmas, 6, 4137–4145, 1999.
4. Chapman, S. C., Watkins, N. W., Dendy, R., Helander, R., and Rowlands, G.: A simple avalanche model as an analogue of magnetospheric activity, Geophys. Res. Lett., 25, 2397–2400, 1998.
5. Chen, J. and Sharma, A. S.: Modelling and prediction of the magnetospheric dynamics during intense geospace storms, J. Geophys. Res., 111, A04209, https://doi.org/10.1029/2005JA011359, 2006.
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