Muon groups and primary composition at 10 to the 13th power to 10 to the 15th power eV

Details Muon groups and primary composition at 10 to the 13th power to 10 to the 15th power eV Muon groups and primary composition at 10 to the 13th power to 10 to the 15th power eV

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....8...24b&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 8 p 24-27 (SEE N85-36066 24-93)

Computer Science

1

Energy Spectra, Monte Carlo Method, Muons, Primary Cosmic Rays, Distribution Functions, Nucleon-Nucleon Interactions, Scintillation Counters, Simulation

Scientific paper

The data on muon groups observed at Baksan underground scintillation
telescope is analyzed. In this analysis we compare the experimental data
with calulations, based on a superposition model in order to obtain the
effective atomic number of primary cosmic rays in the energy range 10 to
the 13th power to 10 to the 15th power eV.

Affiliated with

Also associated with

No associations

Rating

Muon groups and primary composition at 10 to the 13th power to 10 to the 15th power eV 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 Muon groups and primary composition at 10 to the 13th power to 10 to the 15th power eV, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Muon groups and primary composition at 10 to the 13th power to 10 to the 15th power eV will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-759288