Energy spectrum of particles accelerated in the neighborhood of a line of zero magnetic field

Details Energy spectrum of particles accelerated in the neighborhood of a line of zero magnetic field Energy spectrum of particles accelerated in the neighborhood of a line of zero magnetic field

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976sva....19..464b&link_type=abstract

(Astronomicheskii Zhurnal, vol. 52, July-Aug. 1975, p. 763-771.) Soviet Astronomy, vol. 19, no. 4, 1976, p. 464-468. Translatio

Astronomy and Astrophysics

Astronomy

24

Cosmic Rays, Current Sheets, Energy Spectra, Particle Acceleration, Stellar Magnetic Fields, Zero Force Curves, Nonuniform Magnetic Fields, Plasma Turbulence, Pulsars

Scientific paper

The acceleration of charged particles (cosmic rays) in the hyperbolic magnetic and uniform electric fields arising during the decay of a neutral current sheet is examined. It is shown that the acceleration process consists of a direct acceleration by the electric field in the nonadiabatic region near the zero line and a betratron acceleration in the drift region. The characteristic energy of charged particles is determined in the nonrelativistic and ultrarelativistic limits. It is found that the energetic spectra have an exponential form in the high-energy range.

Affiliated with

Also associated with

No associations

Rating

Energy spectrum of particles accelerated in the neighborhood of a line of zero magnetic field 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 Energy spectrum of particles accelerated in the neighborhood of a line of zero magnetic field, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Energy spectrum of particles accelerated in the neighborhood of a line of zero magnetic field will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1299199