Astrophysics and Space Science

, Volume 91, Issue 1, pp 19–33

On the evolution of interacting, magnetized, galactic plasmas

  • Anthony L. Peratt
  • James C. Green

DOI: 10.1007/BF00650210

Cite this article as:
Peratt, A.L. & Green, J.C. Astrophys Space Sci (1983) 91: 19. doi:10.1007/BF00650210


The advent of three-dimensional, electromagnetic, and fully relativistic particle simulations allows a detailed study of a magnetized, rotating plasma, galaxy model. When two such models are simulated, an interaction yielding results resembling observational data from double radio sources, including the emission of synchrotron radiation, are obtained. Simulation derived morphologies, radiation intensities, frequency spectra, and isophote patterns are directly compared to observations. The constituent plasma parameters associated with the source Cygnus A are found to bene=1.8×10−3 cm−3,T=2.8 keV,B=20–30 gamma, with a small population of electrons accelerated to GeV energies by a rotation induced electric field. The results of these simulations, involving a computational resource of five CDC 7600 and five Cray-1 computers, strongly supports an inhomogeneous version of the Klein world model.

Copyright information

© D. Reidel Publishing Co. 1983

Authors and Affiliations

  • Anthony L. Peratt
    • 1
  • James C. Green
    • 2
  1. 1.Intense Particle Beam Theory GroupLos Alamos National LaboratoryLos AlamosUSA
  2. 2.Institute for Plasma ResearchStanford UniversityStanfordUSA