High-Energy Galactic Cosmic Rays

Frank Schroeder,Tareq Abu-Zayyad,Luis A. Anchordoqui, Karen Andeen, Xinhua Bai,Segev BenZvi, D. R. Bergman,Alan Coleman, Hans Dembinski,Michael DuVernois,Thomas K. Gaisser,Francis Halzen,Andreas Haungs,John Kelley,Hermann Kolanoski, Frank McNally,Markus Roth, F. Sarazin, Dave Seckel,Radomir Smida, Dennis Soldin, Delia Tosi

Bulletin of the American Astronomical Society（2019）

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摘要

The origin of the highest energy Galactic cosmic rays is still not understood, nor is the transition to EeV extragalactic particles. Scientific progress requires enhancements of existing air-shower arrays, such as: IceCube with its surface detector IceTop, and the low-energy extensions of both the Telescope Array and the Pierre Auger Observatory.

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