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Bartol Research Institute, University of Delaware, Newark, DE 19716, USA Research Institute, Department of Physics and Astronomy, 217 Sharp Lab, University of Delaware, Newark, DE 19716, USA; Unit for Space Physics, School of Physics, Private Bag X6001, North-West University, Potchefstroom Campus, Potchefstroom, 2520 South Africa Research Institute and Department of Physics and Astronomy, University of Delaware, Newark, DE 19716.
Bartol Research Institute, Department of Physics and Astronomy, University of Delaware, 217 Sharp Laboratory, Newark, DE 19711, USA of Physics, North-West University, Potchefstroom, South Africa
Bartol Research Institute and Department of Physics and Astronomy, University of Delaware, Newark, DE 19716, USA of Physics and Astronomy and the Bartol Research Institute, University of Delaware, Newark, DE 19711, USA Reseach Institute, Department of Physics and Astronomy, University of Delaware, University of Delaware, Newark, DE 19716, USA for Space Physics, North-West University, Potchefstroom, 2520 South Africa for Space Physics, North-West University, Potchefstroom Campus, Potchefstroom, 2520 South Africa University, Unit for Space Physics, Potchefstroom, 2520 South Africa Research Institute, Department of Physics and Astronomy, 217 Sharp Laboratory, University of Delaware, Newark, DE 19716; Also at: Unit for Space Physics, School of Physics, Private Bag X6001, North-West University, Potchefstroom Campus, Potchefstroom, 2520, South Africa.
Unit for Space Physics, School of Physics, Potchefstroom University, Private Bag X6001, Potchefstroom, 2520 South Africa; Bartol Research Institute, University of Delaware, Newark, DE 19716, USA for Space Physics, School of Physics, Potchefstroom University, Potchefstroom, South Afr
A Comparison of Heliospheric Magnetic Fields in the Ab Initio Approach to Cosmic-ray Modulation
Ab Initio Modulation Modeling: The Effect of a Non-Linear Description of Perpendicular Diffusion
Ab Initio Solar Modulation of Cosmic Rays Using Improved Models of Perpendicular Diffusion and Heliospheric Turbulence
Charged Particle Transport in a Non-Uniform Magnetic Field with a Statistically Homogeneous Random Component: Implications for Cosmic-Ray Modulation Models.
Cosmic Ray Modulation: Improving the Agreement Between Modelling and Observations
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