Abstract: The study of the elemental composition and spectra of cosmic rays will provide very crucial clues on the origin of these particles. One of LHAASO aims is to study cosmic rays in a large energy range from 50 TeV to a few of 1 EeV with a consistent calibrated energy scale. At low energy region, it can connect with the direct measurement and get the energy scale of the detectors. At high energy region, it should have enough effective area to reach the UHECRs measurement and transfer the energy scale to the detectors. While it’s hard to cover so large energy range by one type detectors, so experiments are divided into three phases which are in charg
complementarity of cosmic rays and neutrinos in constraining astrophysics in the ultra-high energy r...
Abstract: The main idea of Lomonosov space mission is to study extreme astrophysical phenomena in th...
site is an ideal location for energy spectrum and composition measurements for cosmic rays above 50T...
Abstract: The Cosmic Ray Energetics And Mass (CREAM) instrument is configured with a suite of partic...
Abstract: The flux of cosmic rays above 3×1017 eV has been measured with unprecedented precision at ...
Abstract: An original method of studying chemically etched tracks of heavy nuclei in olivine from pa...
(high resolution space-time pixels) and location (about 600g/cm2 of atmospheric depth) offer a uniqu...
Abstract: The hypothesis is considered that the present, local Galactic cosmic ray spectrum is, due ...
Abstract: We have published the energy spectrum of ultra-high energy cosmic rays (UHECRs) for E> ...
Abstract: The Telescope Array observatory has been collecting ultra high energy cosmic ray data sinc...
Abstract: Recent high precision measurements of the Ultra High Energy Cosmic-ray spectrum have been ...
Abstract: The Pierre Auger Observatory is the world’s largest cosmic ray observatory. Our current ex...
Abstract: The energy spectrum of the cosmic-ray Boron measured by the TRACER experiment at the unpre...
The discovery of cosmic rays with ultra-high energies has opened a window to observe the far and unk...
Abstract: Nearly 50 years ago, the first radio signals from cosmic ray air showers were detected. Af...
complementarity of cosmic rays and neutrinos in constraining astrophysics in the ultra-high energy r...
Abstract: The main idea of Lomonosov space mission is to study extreme astrophysical phenomena in th...
site is an ideal location for energy spectrum and composition measurements for cosmic rays above 50T...
Abstract: The Cosmic Ray Energetics And Mass (CREAM) instrument is configured with a suite of partic...
Abstract: The flux of cosmic rays above 3×1017 eV has been measured with unprecedented precision at ...
Abstract: An original method of studying chemically etched tracks of heavy nuclei in olivine from pa...
(high resolution space-time pixels) and location (about 600g/cm2 of atmospheric depth) offer a uniqu...
Abstract: The hypothesis is considered that the present, local Galactic cosmic ray spectrum is, due ...
Abstract: We have published the energy spectrum of ultra-high energy cosmic rays (UHECRs) for E> ...
Abstract: The Telescope Array observatory has been collecting ultra high energy cosmic ray data sinc...
Abstract: Recent high precision measurements of the Ultra High Energy Cosmic-ray spectrum have been ...
Abstract: The Pierre Auger Observatory is the world’s largest cosmic ray observatory. Our current ex...
Abstract: The energy spectrum of the cosmic-ray Boron measured by the TRACER experiment at the unpre...
The discovery of cosmic rays with ultra-high energies has opened a window to observe the far and unk...
Abstract: Nearly 50 years ago, the first radio signals from cosmic ray air showers were detected. Af...
complementarity of cosmic rays and neutrinos in constraining astrophysics in the ultra-high energy r...
Abstract: The main idea of Lomonosov space mission is to study extreme astrophysical phenomena in th...
site is an ideal location for energy spectrum and composition measurements for cosmic rays above 50T...