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91探花
A CHANDRA image of the supernova remnant Cas A superimposed on the Gemini laser at the UK Central Laser Facility

The plasma physics of supernova remnants in astrophysics is similar to plasma physics of solids irradiated with powerful lasers in the laboratory.

Credit: 1) The Royal Society (personal photo) 2) NASA/CXC/MIT/UMass Amherst/M.D.Stage et al. (Cas A) 3) STFC (laser)

Tony Bell FRS

Academic Visitor

Research theme

  • Particle astrophysics & cosmology
  • Plasma physics

Sub department

  • Atomic and Laser Physics
Tony.Bell@physics.ox.ac.uk
Telephone: 01865 (2)72210
Clarendon Laboratory, room 316.4
  • About
  • Publications

The stability, during formation, of magnetohydrodynamic jets collimated by an azimuthal magnetic field

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 281:1 (1996) 245-256

Authors:

SG Lucek, AR Bell

FOKKER-PLANCK CALCULATIONS WITH IONIZATION DYNAMICS OF SHORT-PULSE LASER-SOLID INTERACTIONS

PHYSICAL REVIEW LETTERS 74:6 (1995) 924-927

Authors:

RPJ TOWN, AR BELL, SJ ROSE

FOKKER-PLANCK SIMULATIONS OF SHORT-PULSE LASER SOLID EXPERIMENTS

LASER INTERACTION WITH MATTER (1995) 145-148

Authors:

RPJ TOWN, AR BELL, SJ ROSE

INTERPLANETARY DIFFUSIVE SHOCK ACCELERATION - EXPONENTIAL OR POWER-LAW SPECTRA

SOLAR PHYSICS 157:1-2 (1995) 349-366

Authors:

M SAVOPULOS, JJ QUENBY, AR BELL

Magnetohydrodynamic jet formation

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 277:4 (1995) 1327-1340

Authors:

AR Bell, SG Lucek

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