Cosmic-ray distribution function with respect to mean free paths in matter

Details Cosmic-ray distribution function with respect to mean free paths in matter Cosmic-ray distribution function with respect to mean free paths in matter

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978izyak..42..914k&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, June 1977.) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheska

Computer Science

Cosmic Rays, Distribution Functions, Mean Free Path, Chemical Composition, Diffusion Coefficient, Energy Spectra, Galactic Nuclei, Halos, Intergalactic Media, Interstellar Gas, Kinetic Energy

Scientific paper

The energy dependence of the ratio of light to intermediate nuclei in cosmic rays is analyzed for disk and central-source models. Source spectra are computed in the diffusion approximation for models with a large quasi-spherical halo. It is shown that the penetration-depth distribution function drops steeply for small mean free paths. The source spectrum of primary nuclei is found to have an approximate power-law dependence on total energy per nucleon.

Affiliated with

Also associated with

No associations

Rating

Cosmic-ray distribution function with respect to mean free paths in matter 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 Cosmic-ray distribution function with respect to mean free paths in matter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmic-ray distribution function with respect to mean free paths in matter will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1297534