Elemental Composition of Cosmic Rays near the Knee by Multiparameter Measurement of Air Showerss

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

29 pages including 10 figures Accepted for publication by Astroparticle Physics, 17th Sept. 1999

Scientific paper

10.1016/S0927-6505(99)00117-6

The small change in the spectral slope of the overall intensity of cosmic rays near 1 PeV may be associated with the endpoint energy of supernova shock acceleration. A crucial test of this connection and other ideas of the origin of the spectral `knee' is the reliable determination of the variation of elemental composition in this region. Recent measurements at the DICE/CASA/MIA air shower installation in Dugway, Utah, USA have provided several independent air shower parameters for each event. The derivation of elemental composition from a combination of Cherenkov size, depth of shower maximum in the atmosphere, muon size and electron size at ground level and the reliability of these results are discussed. There is no evidence from these data for a large change in the mean mass of cosmic rays across the `knee'. These measurements show the cosmic rays are composed of ~ 70% protons and alpha-particles near total energies of 10PeV.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Elemental Composition of Cosmic Rays near the Knee by Multiparameter Measurement of Air Showerss 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 Elemental Composition of Cosmic Rays near the Knee by Multiparameter Measurement of Air Showerss, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Elemental Composition of Cosmic Rays near the Knee by Multiparameter Measurement of Air Showerss will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-153145

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.