WebTitle: HAWC measurements of the energy spectra of cosmic ray protons, helium and heavy nuclei in the TeV range Authors: Juan Carlos Arteaga-Velázquez (for the HAWC Collaboration) Comments: 9 pages, 15 figures, Presented at the 37th International Cosmic Ray Conference (ICRC 2024) Subjects: High Energy Astrophysical Phenomena (astro … WebFeb 22, 2024 · The result of being before one of the most powerful cosmic ray sources discovered so far could be confirmed with the detection of neutrinos from HAWC J1825-134 using neutrino telescopes such as ...
HAWC Science
WebSep 20, 2024 · While HAWC is designed to study the sky in gamma-rays between 500 GeV and 100 TeV, it is also sensitive to showers from primary cosmic rays up to multi-PeV energies. The detector consists of a 22,000 m 2 array of 300 close-packed water Cherenkov detectors (WCDs), each containing 200 kiloliters of purified water and four upward-facing ... WebMar 12, 2024 · Following HAWC observations of the Cygnus Cocoon, massive star-forming regions can now be considered to be sources of very-high-energy (TeV to PeV) Galactic cosmic rays. 24 μm intensity map from Spitzer’s Multiband Imaging Photometer overlaid with TeV gamma-ray map of the Cocoon region from the HAWC observatory. palazzo rospigliosi zagarolo
The cosmic-ray anisotropy with two years of HAWC
WebU.S. Department of Energy Office of Scientific and Technical Information. Search Scholarly Publications. Search terms: Advanced search options Webin HAWC is around 2 deg in radius" Milagro Abdo et al. (2009): - radius: 2.6 +0.7 -0.9 deg Spectral Information: HAWC Abeysekara et al. (2024): - the measured spectrum is relatively hard at 2.2 - the measured spectrum depends on the assumed morphology Flux: Milagro Abdo et al. (2009): WebHAWC: the High-Altitude Water Cherenkov Observatory Cosmic Rays Cosmic Ray Composition Cosmic Ray Energy Spectrum Extensive Air Showers The Earth is immersed in a "sea" of high-energy nuclei known … うどん 三