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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 04/2019, Volume 484, Issue 4, pp. 5755 - 5770
Bow shock pulsar wind nebulae (BSPWNe) are known to show a large variety of shapes and morphologies, both when comparing different objects, and for the same... 
ROTATION | MAGNETOHYDRODYNAMIC SIMULATIONS | ISM: supernova remnants | SPIN-VELOCITY ALIGNMENT | RIEMANN SOLVER | pulsars: general | MHD | PAIR-CREATION | turbulence | methods: numerical | LOW-ALTITUDE | relativistic processes | CRAB-NEBULA | ASTRONOMY & ASTROPHYSICS | RADIO | EMISSION | SCALING LAWS
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 10/2019, Volume 488, Issue 4, pp. 5690 - 5701
Bow shock pulsar wind nebulae are observed with a variety of complex morphologies at different wavelengths, most likely due to differences in the magnetic... 
radiation mechanisms: non-thermal | ISM: supernova remnants | SYNCHROTRON | pulsars: general | MOUSE | X-RAY OBSERVATIONS | methods: numerical | DISCOVERY | relativistic processes | EVOLUTION | ASTRONOMY & ASTROPHYSICS | DYNAMICS | RADIO | polarization | CYGNUS LOOP | TAILS
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2016, Volume 462, Issue 3, pp. 2970 - 2979
Magnetic reconnection is a plasma phenomenon where a topological rearrangement of magnetic field lines with opposite polarity results in dissipation of... 
MHD | Magnetic reconnection | Plasmas | galaxies: jets | Instabilities | plasmas | INSTABILITY | magnetic reconnection | CURRENT SHEETS | FIELD | instabilities | DISCOVERY | GAMMA-RAY FLARES | CRAB-NEBULA | PARTICLE-ACCELERATION | ASTRONOMY & ASTROPHYSICS | JETS | RELATIVISTIC PLASMAS | Physics - High Energy Astrophysical Phenomena
Journal Article
Journal of Geophysical Research: Space Physics, ISSN 0148-0227, 10/2012, Volume 117, Issue A10, p. n/a
Radial diffusion is one of the most important acceleration mechanisms for radiation belt electrons, which can be enhanced from drift‐resonant interactions with... 
radial diffusion coefficient | radiation belt | ULF waves | LFM MHD simulation | ACCELERATION | INNER MAGNETOSPHERE | GEOMAGNETIC STORMS | MAGNETIC STORM | RELATIVISTIC ELECTRONS | FIELD | ASTRONOMY & ASTROPHYSICS | SOLAR-WIND | DYNAMICS | POWER | DRIVEN | Space | Weather | Plasma physics | Magnetism | Models | Atmospheric sciences
Journal Article
Astrophysical Journal, ISSN 0004-637X, 06/2015, Volume 805, Issue 2
We perform 3D relativistic ideal magnetohydrodynamics (MHD) simulations to study the collisions between high-σ (Poynting-flux-dominated (PFD)) blobs which... 
MAGNETIC FIELDS | ELECTROMAGNETIC FIELDS | MAGNETIC RECONNECTION | RESOLUTION | MAGNETOHYDRODYNAMICS | ELECTROMOTIVE FORCE | RELATIVISTIC RANGE | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | ASTROPHYSICS | JETS | TURBULENCE | COSMIC GAMMA BURSTS | GALAXIES | EFFICIENCY | GALAXY NUCLEI | ENERGY LOSSES
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 10/2017, Volume 606, p. A57
Journal Article
IEEE Transactions on Plasma Science, ISSN 0093-3813, 07/2016, Volume 44, Issue 7, pp. 1112 - 1126
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2014, Volume 438, Issue 1, pp. 278 - 306
Journal Article
AIP Conference Proceedings, ISSN 0094-243X, 2014, Volume 1639, Issue 1, pp. 80 - 83
We discuss the incorporation of relativistic modeling capabilities into the PERSEUS extended MHD simulation code for high-energy-density (HED) plasmas, and... 
PLASMA DENSITY | LASERS | PLASMA SIMULATION | ELECTRON BEAMS | RELAXATION | MAGNETOHYDRODYNAMICS | ENERGY DENSITY | LINEAR PINCH DEVICES | COMPUTERIZED SIMULATION | RELATIVISTIC RANGE | ACCELERATION | 70 PLASMA PHYSICS AND FUSION TECHNOLOGY | PLASMA | P CODES
Conference Proceeding
Astrophysics and Space Science, ISSN 0004-640X, 4/2009, Volume 320, Issue 1, pp. 107 - 114
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 08/2017, Volume 469, Issue 4, pp. 4957 - 4978
Relativistic jets in active galactic nuclei (AGN) convert as much as half of their energy into radiation. To explore the poorly understood processes that are... 
SPATIAL GROWTH | MAGNETOHYDRODYNAMIC SIMULATIONS | RAY BURST JETS | magnetic fields | galaxies: jets | BLACK-HOLE SPIN | MHD | AFTERGLOW LIGHT CURVES | RELATIVISTIC MHD SIMULATIONS | instabilities | NUMERICAL SCHEME | GAMMA-RAY | galaxies: active | ASTRONOMY & ASTROPHYSICS | CURRENT-DRIVEN INSTABILITY | SUPERLUMINAL MOTION
Journal Article