Physics of the Cosmos
Exploring fundamental questions regarding the physical forces of the universe

Cosmic Ray and Neutrino Science Interest Group
(CR SIG)

Image: Jelly Fish Nebula (IC 443) source of cosmic rays. Credit: NASA / DOE / Fermi LAT Collaboration, NOAO / AURA / NSF, JPL-Caltech/UCLA

The goals of the Cosmic Ray and Neutrino Science Interest Group (CR SIG) are to provide quantitative metrics and assessments to NASA in regard to current and future needs of the cosmic-ray astrophysics community and to act as a focal point and forum for the cosmic ray community.

CR SIG will work towards producing a white paper covering:

  • the major open science questions
  • a brief survey of the current and planned, US and International, space and ground-based projects — their energy coverage (from about 108 eV to 102 eV), sky coverage, and particle type coverage (electrons, positrons, nucleons, anti-nucleons, nuclei, anti-nuclei, neutrinos, and new particles)
  • a survey of the state-of-the-art capabilities, the next generation technology needs, and potential science return from new technologies and capabilities
  • a vision for the future of cosmic ray science in space

The CR SIG is open to the scientific community.

If you are interested in contributing to the work of the CR SIG, please subscribe using the link below.


Subscribe to the
Cosmic Ray and Neutrino SIG News and Announcements Email List.

News
31 March 2025
Next HWO Seminar Series Talks on 2 April 2025
»  Details
NASA Scientific Balloon Program Flight Opportunity
»  Details
Save the Date: AXIS Community Science Conference: 14 – 16 May 2025
»  Details
Chandra/CIAO Workshop at UMass Lowell 19-23 May 2025; Register by 25 April 2025
»  Details
Recent changes to NASA Science Advisory Committees — Impact on NASA Program Analysis Groups
»  Details