Energy Spectrum and Chemical Composition of Cosmic Rays Determined with the HEGRA Arrays

Details Energy Spectrum and Chemical Composition of Cosmic Rays Determined with the HEGRA Arrays Energy Spectrum and Chemical Composition of Cosmic Rays Determined with the HEGRA Arrays

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000nva..conf..311c&link_type=abstract

NEW VISTAS IN ASTROPHYSICS. Proceedings of the International School of Cosmic Ray Astrophysics 20th Anniversary, 11th Course. He

Astronomy and Astrophysics

Astrophysics

Scientific paper

The HEGRA scintillator and Cherenkov light counters allow to determine the energy and coarse chemical composition of charged cosmic rays in the energy range between 1014 eV and 1016 eV. The energy spectrum obtained from HEGRA data shows a gradual steepening around 3 PeV. No abrupt change in the chemical composition is noticeable.

Affiliated with

Also associated with

No associations

Rating

Energy Spectrum and Chemical Composition of Cosmic Rays Determined with the HEGRA Arrays 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 Spectrum and Chemical Composition of Cosmic Rays Determined with the HEGRA Arrays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Energy Spectrum and Chemical Composition of Cosmic Rays Determined with the HEGRA Arrays will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-764348