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Cosmic Ray Models

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اقرأ أكثر حفظ في قائمتي
  • معلومة اضافية
    • Contributors:
      AstroParticule et Cosmologie (APC (UMR_7164)); Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris; Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
    • بيانات النشر:
      CCSD
      Pergamon Press
      Elsevier [1978-.]
    • الموضوع:
      2019
    • Collection:
      Archive de l'Observatoire de Paris (HAL)
    • نبذة مختصرة :
      International audience ; We review progress in high-energy cosmic ray physics focusing on recent experimental results and models developed for their interpretation. Emphasis is put on the propagation of charged cosmic rays, covering the whole range from ∼ (20–50) GV, i.e. the rigidity when solar modulations can be neglected, up to the highest energies observed. We discuss models aiming to explain the anomalies in Galactic cosmic rays, the knee, and the transition from Galactic to extragalactic cosmic rays.
    • Relation:
      info:eu-repo/semantics/altIdentifier/arxiv/1904.08160; ARXIV: 1904.08160; INSPIRE: 1730269
    • الرقم المعرف:
      10.1016/j.ppnp.2019.07.002
    • الدخول الالكتروني :
      https://hal.science/hal-02136889
      https://hal.science/hal-02136889v1/document
      https://hal.science/hal-02136889v1/file/S0146641019300456.pdf
      https://doi.org/10.1016/j.ppnp.2019.07.002
    • Rights:
      http://creativecommons.org/licenses/by-nc/ ; info:eu-repo/semantics/OpenAccess
    • الرقم المعرف:
      edsbas.E2DF1B30