Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Unit for Space Physics, Potchefstroom University, Potchefstroom, South Africa
Centre for Space Research, North-West University, Potchefstroom Campus, Private Bag X6001, Potchefstroom 2520, South Africa
North-West University, Unit for Space Physics North-West University, Potchefstroom, NW 2520 South Africa Univ., Tucson, AZ
Unit for Space Physics, School of Physics, Private Bag X6001, North-West University, Potchefstroom Campus, Potchefstroom, 2520 South Africa University, Unit for Space Physics North-West University, Potchefstroom, 2520 Research Unit, Department of Physics, Potchefstroom University for CHE, 2520 Potchefstroom, South Africa
Space Research Unit, Department of Physics, Potchefstroom University for CHE 2520 Potchefstroom, South Africa
Unit for Space Physics, School of Physics, North-West University, Potchefstroom, South Africa
Unit for Space Physics, Potchefstroom University for CHE, 2520 Potchefstroom, South Africa
Bartol Research Institute, University of Delaware, USA
Unit for Space Physics, School of Physics, North-West University, Potchefstroom Campus, Private Bag X6001, Potchefstroom, 2520 South Africa for Space Physics, North-West University, Potchefstroom, 2520 South Africa University for Christian Higher Education; South African Council for Scientific and Industrial Research, Cosmic Ray Research Unit, Republic of South Africa
Center for Space Research, North-West University, 2520 Potchefstroom, South Africa.
Unit for Space Physics, Potchefstroom Campus of the North-West University, Venter Street, Potchefstroom 2520, South Africa University for Christian Higher Education, Republic of South Africa
North-West University, Potchefstroom Campus, Potchefstroom, 2520, South Africa of Physics, Potchefstroom University for CHE, Potchefstroom, South Africa
Space Research Unit Department of Physics,
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 Comparison of Heliospheric Magnetic Fields in the Ab Initio Approach to Cosmic-ray Modulation
A comparison of predictions of a wavy neutral sheet drift model with cosmic-ray data over a whole modulation cycle - 1976-1987
A Fisk-Parker Hybrid Heliospheric Magnetic Field With a Solar-Cycle Dependence
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