Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
Center for Space Plasmas and Aeronomic Research, University of Alabama in Huntsville, 320 Sparkman Drive, Huntsville, AL 35805, USA
CSPAR, University of Alabama, Huntsville, Alabama 35805, USA
University Bochum, Theoretische Physik IV Ruhr-Universität Bochum 44780 Bochum Germany, Bochum, 44780, Germany
Institut für Theoretische Physik, Lehrstuhl IV: Weltraum- und Astrophysik, Ruhr-Universität Bochum, D-44780 Bochum, Germany
Institut für Theoretische Physik, Lehrstuhl IV: Weltraum und Astrophysik, Ruhr-Universität Bochum, D-44780 Bochum, Germany
Cosmic ray perpendicular diffusion coefficients calculated from the Newton-Lorentz equation
Diffusive shock acceleration at interplanetary perpendicular shock waves: Influence of the large scale structure of turbulence on the maximum particle energy
Magnetic-field-line random walk in turbulence: A two-point correlation function description
Nonlinear Guiding Center Theory of Perpendicular Diffusion: Derivation from the Newton-Lorentz Equation
Numerical investigation of the cosmic-ray scattering anisotropy and Bohm diffusion in space plasmas
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