Scaling of the geomagnetic indices and solar wind: a Fokker-Planck approach Bogdan A. Hnat Collaborators: S. C. Chapman and G. Rowlands; University of.
Analysis of financial data on different timescales - and a comparison with turbulence Robert Stresing Andreas Nawroth Joachim Peinke EURANDOM 6-8 March.
Dynamics of Complex Systems M.Y. Choi Department of Physics Seoul National University Seoul 151-747, Korea May 2005 PITP Conference Main Collaborators.
SES 2007 A Multiresolution Approach for Statistical Mobility Prediction of Unmanned Ground Vehicles 44 th Annual Technical Meeting of the Society of Engineering.
Cosmic Ray (CR) transport in MHD turbulence Huirong Yan Kavli Institute of Astronomy & Astrophysics, Peking U.
Influence of turbulence on the dynamo threshold B. Dubrulle, GIT/SPEC N. Leprovost, R. Dolganov, P. Blaineau J-P. Laval and F. Daviaud.
1 The Kinetic Basis of Molecular Individualism and the Difference Between Ellipsoid and Parallelepiped Alexander Gorban ETH Zurich, Switzerland, and Institute.
Practical Models of Solar Energetic Particle Transport Leon Kocharov Space Research Laboratory University of Turku, Finland Requirements.
A new algorithm for the kinetic analysis of intra-beam scattering in storage rings. P.R.Zenkevich*,O. Boine-Frenkenheim**, A. Ye. Bolshakov* *ITEP, Moscow,
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University of Catania INFN-LNS Heavy flavor Suppression : Langevin vs Boltzmann S. K. Das, F. Scardina V. Greco, S. Plumari.
F. Scardina University of Catania INFN-LNS Heavy Flavor in Medium Momentum Evolution: Langevin vs Boltzmann V. Greco S. K. Das S. Plumari V. Minissale.