Estimation of the energy spectrum of cosmic ray electrons at the atmospheric depth (3.8 7.4)g.cm-2

Details Estimation of the energy spectrum of cosmic ray electrons at the atmospheric depth (3.8 7.4)g.cm-2 Estimation of the energy spectrum of cosmic ray electrons at the atmospheric depth (3.8 7.4)g.cm-2

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999czjph..49.1503s&link_type=abstract

Czechoslovak Journal of Physics, vol. 49, Issue 10, p.1503-1507

Physics

Scientific paper

Analytical calculations have been done to estimate the energy spectra of the secondary electrons originated from the decay of charged and neutral pions initiated on the upper atmosphere from the primary nucleon-air interactions in the energy range (4-100) GeV. The calculations are valid up to an atmospheric depth of about (3.8-7.4) g.cm-2. The derived results are compared with the observed electron fluxes available from the balloon flight experiments of MASS2, HEAT, magnetic spectrometer system of Golden et al., instrument using scintillating fibers of Nishimura et al., and BETS.

Affiliated with

Also associated with

No associations

Rating

Estimation of the energy spectrum of cosmic ray electrons at the atmospheric depth (3.8 7.4)g.cm-2 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 Estimation of the energy spectrum of cosmic ray electrons at the atmospheric depth (3.8 7.4)g.cm-2, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Estimation of the energy spectrum of cosmic ray electrons at the atmospheric depth (3.8 7.4)g.cm-2 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1084580