HelioWebKatholieke University of Leuven, Astronomical Institute
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I[Katholieke University of Leuven, Astronomical Institute]
PI["Parent Institutions (1)"]
CI["Child Institutions (0)"]
AW["Affiliated Works (89)"]
CA["Linked Collaborating Authors (15)"]
I== skos:broader ==>PI
CI== skos:broader ==>I
AW== affil ==>I
AW== author ==>CA
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Child Institutions [?]
Affiliated Works
sorted by decreasing year, and then by display-name
- Numerical Simulations of the Jovian Magnetosphere: Influence of the Solar Wind
- Dipolarization Front: A Distinctive Feature of the Reconnection Onset in the Magnetotail
- Disentangling the Magnetic Flux Rope Topology From Coronal Mass Ejections
- Experimental onset threshold and magnetic pressure pileup for 3D Sweet-Parker reconnection
- Implicit PIC Simulations of Magnetic Guide-Field Reconnection*
- Kinetic Simulations of Magnetic Reconnection in the Geomagnetic tail with Oxygen, Using Physical Mass Ratios
- Linear and non linear tearing and Kelvin-Helmholtz driven instabilities in current-sheets with velocity shears: three-dimensional compressive MHD simulations.
- Non-Steady Reconnection In Stratified Atmospheres: Applications To The Solar Environment
- Onset and non-steady state evolutions of collisionless magnetic reconnection
- 3d Flux Rope Dynamics Including Reconnection, Bouncing, And Guide Field Compression
- Can Electron Phase-Space Holes Help a Spacecraft Locate its Position in the Geometry of Guide-Field Reconnection?
- Global MHD simulations of Jupiter's magnetosphere: study of the ionosphere-magnetosphere coupling
- Model of Electron Pressure Anisotropy in the Process of Magnetic Reconnection
- Spontaneous non-steady reconnection within the framework of pure resistive magnetohydrodynamics: is anomalous resistivity really unescapable?
- 0.5 - 165 MeV proton and 102 - 312 keV electron injections during the 2006 December 13 SEP event
- Coupling global and kinetic scales with the implicit Particle-in-Cell methods
- Electron diffusion region scalings in antiparallel magnetic reconnection
- Laboratory Investigations of Impulsive Dynamics Of Flux Ropes In 3D
- Nature of the Magnetic Fields in Magnetic Clouds: Twist or Writhe?
- Observational and numerical study of the 25 July 2004 event
- Realistic Particle-in-Cell simulations of the two-component solar wind
- Spontaneous and chaotic fast reconnection in three dimensional current-sheets (Invited)
- VOs and Heliophysics: Would anyone like some CASSIS?
- 3-D Implicie-PIC Simulation Studies of Electrid Fields During Magnetic Reconnection
- Developing a new model for gradual SEP events: Peak intensities and fluences within 1.6 AU
- First Reconnected Flux Tubes
- Inhomogeneous Two-Stream Instability and Electron Holes near the Magnetic-Reconnection Separatrix
- Investigating the Origins and Heliospheric Evolution of Homologous CMEs Originating from NOAA AR11093 on 7 and 14 August 2010
- Multi-Spacecraft Reconstruction of the Magnetic Fields InICMEs with Writhe Structure
- 3D Implicit Particle-in-Cell Simulations of Solar Wind - Body Interactions
- Evidence of Multiple X-lines in the Solar Wind from Overlapping Hall Magnetic Fields
- Influence of the interplanetary shock on the radial dependence of solar energetic particle intensities
- Magnetic Field Structure in ICMEs: Comparison and Validity of Different Models
- Numerical modeling of the initiation of coronal mass ejections in active region NOAA 9415
- Structure of Dipolarization Front at Reconnection Point in 3D PIC simulations
- The role of streamers in the deflection of coronal mass ejections: comparison between STEREO 3D reconstructions and numerical simulations
- 3D Electromagnetic Particle-in-Cell simulations of the solar wind interaction with lunar magnetic anomalies
- Global Simulations of the Magnetosphere under Sub-Alfvénic Solar Wind Conditions. (Invited)
- Helioseismology in a bottle: an experimental technique
- Ion kinetic structure of dipolarization fronts created by magnetic reconnection
- Numerical Ideal MHD Modeling of the Kink Double-Gradient Magnetic Instability
- On the Importance of Kinetic Effects on Electron Acceleration near the Reconnection Region
- On the Influence of the Solar Wind Density on the Jovian Main Auroral Emission
- Spacecraft-environment interaction model cross comparison applied to Solar Probe Plus
- The Evolution of the Global Coronal Shock in the June 7, 2011 Event: An MHD Simulation Study
- Using Multi-Spacecraft Technique to Identify the Structure of Magnetic Field in CMEs
- Whistlers Associated With Electron Phase Space Holes During Magnetic Reconnection In The Magnetotail
- Electromagnetic Particle-in-Cell Simulations of the Solar Wind Interaction with Lunar Magnetic Anomalies: Ion and Electron Dynamics Under Varying Solar Wind Conditions.
- Implication of Kappa models in realistic parameterization of the kinetic anisotropy and the resulting instabilities in space plasmas
- Jupiter's Main Auroral Emission for Different Solar Wind Conditions
- Kinetic Effects in Parametric Instabilities of Finite Amplitude Alfven Waves in a Drifting Multi-Species Plasma
- Three-Dimensional Magnetic Reconnection Under Low Chromospheric Conditions Using a Two-Fluid Weakly Ionized Reactive Plasma Model
- Mixing of Proton and Electron Scales - Effects of Proton Temperature Anisotropy on the Electron Firehose Instability
- Multifluid Modeling of the Partially Ionized Chromosphere with Effects of Impact Ionization, Radiative Recombination and Charge Exchange
- Null Points in Three-Dimensional Kinetic Simulations of Magnetic Reconnection
- Partially Ionized Plasma Three-Fluid Modeling of Magnetic Reconnection in the Sun Chromosphere
- Solar Wind Modelling: MHD And Kinetic Treatments with Kappa Distributions for the Electrons
- Solar wind driven instability with non-Maxwellian distribution functions
- Three-Fluid collisional and reactive magnetic reconnection with radiative effects in chromospheric conditions
- Two-fluid Modeling of Drift Waves in the Solar Atmosphere
- Twofluid Simulations of Propagation of Slow and ALFVÉN Waves in the Partially Ionized Solar Chromosphere
- Comparison between Magnetopause and Magnetotail Reconnection Processes
- Electron Heating and Acceleration in a Reconnecting Magnetotail
- Global Particle-in-Cell Simulations of Mercury's Magnetosphere
- Modeling of Jovian Auroral Polar Ion and Proton Precipitation
- Nonlinear Evolution of Observed Fast Streams in the Solar Wind - Micro-instabilities and Energy Exchange between Protons and Alpha Particles
- Particle Acceleration and Heating Processes at the Dayside Magnetopause
- Turbulence generated by reconnection jets collision
- 2.5D Numerical simulations of ICMES up to 1AU.
- More on the internal structure of Coronal Magnetic Eruptions
- Observation-based Sun-to-Earth simulations of geo-effective Coronal Mass Ejections with EUHFORIA
- Suprathermal particles in the solar wind self-regulation
- A collaborative study of the Hermean magnetosphere using the multiple numerical and visualization techniques of the SHOTS project
- A study of the role of CME-CME interactions on CME geo-effectiveness with EUHFORIA
- Auroral diagnosis of solar wind interaction with Jupiter's magnetosphere
- Data-driven and observation-based modeling of CMEs in the inner heliosphere with EUHFORIA
- Developing Fast Solar Wind Modeling with EUHFORIA
- EUV Observations of the Middle Corona From the L5 Perspective
- Improving Modelling Areas of Open-Closed Flux in the Corona Using Remote Sensing Observations
- Locking Degree for the Chilean subduction zone and its link to spatio-temporal evolution of deformation and seismicity
- Solar energetic particles experience EUHFORIA's CMEs in PARADISE
- CME-CME Interactions as Sources of CME Helio-Effectiveness: the Early September 2017 Events
- Collisional and Reactive Multi-fluid Modeling of Acoustic Wave Propagation and Heating in Gravitationally Stratified Chromospheric plasma
- Critical factors affecting change in CME orientation
- Implementing the MULTI-VP Coronal Model in EUHFORIA: Results and Comparisons with the WSA Coronal Model
- Low-Temperature Gas-Phase Rate Coefficients: Measurements, Theory, and Astrochemical Modeling.
- Modelling energetic particles in the vicinity of high-speed solar wind streams with PARADISE
- Real time physics-based solar wind forecasts for SafeSpace
- Using InSight Wind Data to Validate Atmospheric Models and Improve Predictions for Other Locations on Mars