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Magnetic field reversals and secular variation in a bistable geodynamo model. Physics of the Earth and Planetary Interiors 43.
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A model of heat and mass transfer in a porous cometary nucleus based on a kinetic treatment of mass flow. Icarus 45.
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Stability of water ice under a porous nonvolatile layer: implications to the south polar layered deposits of Mars. Planetary and Space Science 46.
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Noise reduction in helioseismic power spectra by non-orthogonal wavelets. Astronomy and Astrophysics 47.
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On cyclotron wave heating and acceleration of solar wind ions in the outer corona. Journal Geophysical Research 50.
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A semi-kinetic model of wave-ion interaction in the solar corona. Geophysical Research Letters 51.
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Partcile simulation of collsionless magnetic reconnection in the harris model. In: Space Plasma Simulation, pp. 233 - 235 (Eds. 56.
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Spectral windows of the solar atmosphere. In: Proc. ``Solar Encounter: The First Solar Orbiter Workshop'', (ESA SP-493), pp. 199 - 203 (Eds. Battrick, B.; Sawaya-Lacoste, H.). ESA Publ. Div., Noordwijk (2001)
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Particle simulation of magnetic reconnection using TRISTAN. In: Space Plasma Simulation, pp. 275 - 278 (Eds. 58.
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Numerical Techniques - Vizualisation of three-dimensional plasma dynamics. In: Space Plasma Simulation, pp. 177 - 179 (Eds. 59.
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Linear theory and simulation of current sheet instabilities. In: Space Plasma Simulation, pp. 352 - 355 (Eds.