Energy-dependent diffusion of cosmic rays in the dynamical halo model

Details Energy-dependent diffusion of cosmic rays in the dynamical halo model Energy-dependent diffusion of cosmic rays in the dynamical halo model

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...237..814k&link_type=abstract

Astrophysical Journal, Part 1, vol. 237, May 1, 1980, p. 814-818.

Physics

Nuclear Physics

18

Astronomical Models, Cosmic Rays, Milky Way Galaxy, Nuclei (Nuclear Physics), Particle Diffusion, Dynamic Models, Energy Spectra, Interplanetary Medium, Mathematical Models, Proton Energy, Runge-Kutta Method

Scientific paper

A simple Runge-Kutta method is used to obtain exact numerical results for the energy-dependent diffusion of galactic cosmic-ray nuclei in the dynamical halo model. A new observational limit on the galactic modulation parameter q = VD/K is obtained from the demodulated interplanetary proton observations. The numerical results are compared with the approximate analytic solutions of Jokipii and Jones.

Affiliated with

Also associated with

No associations

Rating

Energy-dependent diffusion of cosmic rays in the dynamical halo model 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-dependent diffusion of cosmic rays in the dynamical halo model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Energy-dependent diffusion of cosmic rays in the dynamical halo model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1358898