Results from the KASCADE, KASCADE-Grande, and LOPES experiments

Abstract

The origin of high-energy cosmic rays in the energy range from 10^14 to 10^18 eV is explored with the KASCADE and KASCADE-Grande experiments. Radio signals from air showers are measured with the LOPES experiment. An overview on results is given.

Talk at The ninth International Conference on Topics in Astroparticle and Underground Physics, TAUP 2005, Zaragoza, September 10-14, 2005

References in corpus (8)

• KASCADE measurements of energy spectra for elemental groups of cosmic rays: Results and open problems
• High-energy particle acceleration in the shell of a supernova remnant
• Detection and imaging of atmospheric radio flashes from cosmic ray air showers
• Models of the Knee in the Energy Spectrum of Cosmic Rays
• Radio emission from cosmic ray air showers: simulation results and parametrization
• Search for cosmic-ray point sources with KASCADE
• Primary Proton Spectrum of Cosmic Rays measured with Single Hadrons
• Geometric structures in hadronic cores of extensive air showers observed by KASCADE

Cited by in corpus (6)

• Cosmic rays from the knee to the second knee: 10^14 to 10^18 eV
• Bottom-up Acceleration of Ultra-High-Energy Cosmic Rays in the Jets of Active Galactic Nuclei
• Acceleration of Heavy Ions at Non-Relativistic Collisionless Shocks
• Revisiting Propagation Delays of Ultra-High-Energy Cosmic Rays from Long-lived Sources
• Theory of nonlinear particle acceleration at shocks and self-generation of the magnetic field
• Espresso Acceleration of Ultra-High-Energy Cosmic Rays up to the Hillas Limit in Relativistic MHD Jets