The spectrum of particles radiating in cylindrical and filament magnetic fields

Details The spectrum of particles radiating in cylindrical and filament magnetic fields The spectrum of particles radiating in cylindrical and filament magnetic fields

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...334..841p&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 334, Nov. 15, 1988, p. 841-851.

Astronomy and Astrophysics

Astrophysics

Charged Particles, Energy Distribution, Magnetic Field Configurations, Particle Energy, Particle Motion, Trajectory Analysis, Crab Nebula, Filaments, Magnetohydrodynamics, Particle Acceleration, Supernova Remnants

Scientific paper

Particle trajectories, and the energy distribution and frequency spectrum for an initially power-law distribution of particle energies, are calculated for particles radiating in cylindrical and filament magnetic fields. If there is a continuous supply of particles to the fields, the spectrum develops two "breaks". For the filament field the spectral index changes from -α at low frequencies to -α - 0.875 at high frequencies. There is also a cutoff to the spectrum. The results are applied to Cas A and the Crab Nebula.

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