Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..269b&link_type=abstract
(Pis'ma v Astronomicheskii Zhurnal, vol. 10, Apr. 1984, p. 269-274) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, Mar.-Apr
Astronomy and Astrophysics
Astronomy
1
Energetic Particles, Galactic Cosmic Rays, Galactic Nuclei, Milky Way Galaxy, Neutron Flux Density, Astronomical Models, Magnetic Rigidity, Particle Trajectories, Supernovae
Scientific paper
An analysis of the motion of particles in a magnetic field within the galactic center and extending to the spiral arms is performed as a test of the center being possibly the source of observed 10,000-100,000 TeV cosmic rays. Particles with rigidities exceeding 10,000 TV are shown to be little influenced by the galactic magnetic field. Trajectories are therefore calculated for such particles, with the magnetic field being concentrated along the spiral arms. The particles are traced until escaping from the halo. It is found that anisotropy will be breached in the solar neighborhood, which disagrees with observed particle counts. It is suggested that consideration be given to supernovae and extragalactic origins for the high energy cosmic rays.
Berezinskij V. S.
Mikhajlov A. A.
No associations
LandOfFree
Can the ultrahigh-energy cosmic rays STEM from the galactic center? does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Can the ultrahigh-energy cosmic rays STEM from the galactic center?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Can the ultrahigh-energy cosmic rays STEM from the galactic center? will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1501119