Physics
Scientist
Unit for Space Physics, Potchefstroom University, Potchefstroom, South Africa
Unit for Space Physics, School of Physics, North-West University, Potchefstroom, South Africa
Centre for Space Research, North-West University, 2520 Potchefstroom, South Africa
Unit for Space Physics, School of Physics, North-West University, 2520 Potchefstroom, South Africa for Space Physics, Potchefstroom University for CHE, 2520 Potchefstroom, South Africa
Unit for Space Physics, Potchefstroom University for CHE, South Africa
Unit for Space Physics, North-West University, 2520 Potchefstroom, South Africa
Center for Space Research, North-West University, 2520 Potchefstroom, South Africa.
Unit for Space Physics, School of Physics, Potchefstroom University, Potchefstroom, South Africa
Unit for Space Physics, North-West University 2520, Potchefstroom, South Africa for Space Physics, School of Physics, Potchefstroom University for CHE, 2520 Potchefstroom, South Africa for Space Physics, North-West University, 2520, Potchefstroom, South Africa
Unit for Space Physics, School of Physics, Potchefstroom University for C.H.E., 2520 Potchefstroom, South Africa
Unit for Space Physics, School of Physics, North-West University, 2520 Potchefstroom, South Africa
Unit for Space Physics, North-West University, 2520 Potchefstroom, South Africa for Space Physics, School of Physics, Potchefstroom University for Christian Higher Education, 2520 Potchefstroom, South Africa for Space Physics, Potchefstroom University, 2520 Potchefstroom, South Africa
Institut für Theoretische Physik IV, Ruhr-Universität Bochum, 44780 Bochum, Germany
Unit for Space Physics, School of Physics, North-West University, 2520 Potche
3-20 MeV Electrons in the Inner Three-dimensional Heliosphere at Solar Maximum: Ulysses COSPIN/KET Observations
3-20 MeV Electrons in the Inner Three-dimensional Heliosphere at Solar Maximum: Ulysses COSPIN/KET Observations.
A heliospheric hybrid model: hydrodynamic plasma flow and kinetic cosmic ray transport
A new cosmic ray modulation model for the 11-year and 22-year cycles
An overview of Jovian electrons during the distant Ulysses Jupiter flyby
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