Energy spectra of proton and nuclei of primary cosmic rays in energy region 10 TeV/particle

Details Energy spectra of proton and nuclei of primary cosmic rays in energy region 10 TeV/particle Energy spectra of proton and nuclei of primary cosmic rays in energy region 10 TeV/particle

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6..228m&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 228-231 (SEE N85-35848 24-93)

Computer Science

Chemical Composition, Cosmic Ray Showers, Energy Spectra, Nuclear Emulsions, Primary Cosmic Rays, Depth, Nuclear Interactions, Stratosphere, Zenith

Scientific paper

To investigate the chemical composition of primary cosmic rays, several emulsion chambers were exposed at a 10.8 g/sq cm. depth in the stratosphere. Each chamber has the area of 0.92x0.46 sq m. and the depth of 14 c.u. The exposure time of chambers processed by now is 260 hours. The detecting layers were X-ray films and nuclear emulsions, which allowed to measure an energy of cascade and a type of primary particle. Results and techniques are described.

Affiliated with

Also associated with

No associations

Rating

Energy spectra of proton and nuclei of primary cosmic rays in energy region 10 TeV/particle 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 spectra of proton and nuclei of primary cosmic rays in energy region 10 TeV/particle, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Energy spectra of proton and nuclei of primary cosmic rays in energy region 10 TeV/particle will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-758136