HelioWebPotchefstroom University for Christian Higher Education, School of Physics
flowchart
I[Potchefstroom University for Christian Higher Education, School of Physics]
PI["Parent Institutions (1)"]
CI["Child Institutions (0)"]
AW["Affiliated Works (41)"]
CA["Linked Collaborating Authors (1)"]
I== skos:broader ==>PI
CI== skos:broader ==>I
AW== affil ==>I
AW== author ==>CA
click PI "#parent-institutions"
click CI "#child-institutions"
click AW "#affiliated-works"
click CA "#collaborating-authors"
Parent Institutions [?]
Child Institutions [?]
Affiliated Works
sorted by decreasing year, and then by display-name
- 3-20 MeV Electrons in the Inner Three-dimensional Heliosphere at Solar Maximum: Ulysses COSPIN/KET Observations.
- Improved Representation of Heliospheric Magnetic Field Fluctuations in Ab Initio Models of Cosmic Ray Modulation
- The Effect of a Fisk-type Heliospheric Magnetic Field on Cosmic Ray Modulation
- Ab Initio Modulation Modeling: The Effect of a Non-Linear Description of Perpendicular Diffusion
- Multiple Balloon Campaign (MINIS) to Study MeV Electron Precipitation
- Self Consistent Modeling of Turbulence Transport with Implications for Cosmic Ray Transport and Modulation
- Transport Parameters in the Heliosphere Inferred from Observed Cosmic Ray Spectra
- A Calibrated Neutron Monitor Network
- A Comparison of Heliospheric Magnetic Fields in the Ab Initio Approach to Cosmic-ray Modulation
- A Multiple Balloon Campaign to Study Relativistic Electron Loss Mechanisms
- Ab Initio Solar Modulation of Cosmic Rays Using Improved Models of Perpendicular Diffusion and Heliospheric Turbulence
- Cosmic Ray Modulation: Improving the Agreement Between Modelling and Observations
- Effect of Latitudinal Dependence of Boundary Conditions on Transport of Turbulence in the Heliosphere
- Radial evolution of cross helicity in the solar wind at high latitudes: Ulysses observations and turbulence modeling results
- Charged Particle Transport in a Non-Uniform Magnetic Field with a Statistically Homogeneous Random Component: Implications for Cosmic-Ray Modulation Models.
- Direct Observation of Prompt Solar Flare Perturbation to Stratospheric Electrodynamics
- Effects of Perpendicular Diffusion in the Radial Direction on the Acceleration of Particles at the Solar Wind Termination Shock
- Effects of the January 16th-20th Solar Flares on the Fair Weather Global Electric Circuit.
- Global Monitoring of Relativistic Electron Precipitation with Balloon Networks: MINIS and Beyond
- Investigating EMIC waves as a relativistic electron precipitation mechanism during the MINIS balloon campaign
- Ionospheric convection observations following the solar flare of 20 January 2005 and during the geomagnetic storm of 21 January 2005
- MINIS Balloon and RHESSI Observations of a Solar Energetic Particle Event
- MINIS Observations of MeV electron precipitation on January 21st 2005
- Solar neutron events associated with large solar flares in solar cycle 23
- The Effect of Turbulence at Small Wavenumbers on Particle Diffusion
- The Effect of a Fisk-Parker Hybrid Magnetic Field on 26-day Recurrent Cosmic-Ray Variations
- BARREL: A Balloon Array for Monitoring Relativistic Electron Losses during the RBSP Mission
- Influence of Magnetic Turbulence on Charged Particle Drift
- Recurrent Cosmic-ray Variations as a Probe of the Heliospheric Magnetic Field
- Three Dimensional Time Dependent Stochastic Method for Cosmic-ray Modulation
- Calculation of Drift and Diffusion Coefficients for Cosmic Rays inside the Heliospheric Termination Shock
- Stochastic Simulation of Galactic Cosmic Ray Modulation with 3D Wavy Heliospheric Current Sheet Drifts at Solar Minimum
- On Cosmic Ray Modulation in the Heliosheath and beyond the Heliopause
- Implications of composite turbulence transport for cosmic-ray modulation
- Modelling cosmic ray propagation in the heliosheath and beyond
- Remarks on the Implementation of Neutral Sheet Drift in Cosmic-Ray Modulation Models
- The transport of cosmic rays in the heliosheath
- A Comparison of Cosmic-Ray Modulation During the 1986- and 2009 Solar Minima
- Perpendicular diffusion: Variations on the NLGC theme
- Transport of cosmic rays across the heliopause
- Analysis of Voyager 1 Magnetic Field Data From 1977 to 1990