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Measurements and implications of cosmic ray anisotropies from TeV to trans-EeV energies

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F19%3A00539839" target="_blank" >RIV/68378271:_____/19:00539839 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1016/j.astropartphys.2018.08.005" target="_blank" >https://doi.org/10.1016/j.astropartphys.2018.08.005</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.astropartphys.2018.08.005" target="_blank" >10.1016/j.astropartphys.2018.08.005</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Measurements and implications of cosmic ray anisotropies from TeV to trans-EeV energies

  • Original language description

    Important observational results have been recently reported on the angular distributions of cosmic rays at all energies, calling into question the perception of cosmic rays a decade ago. These results together with their in-progress interpretations are summarized in this review paper, covering both large-scale and small-scale anisotropies from TeV energies to the highest ones. While the magnetic field in the Galaxy has long been considered as an external data imprinting a quasi-random walk to particles and thus shaping the angular distributions of Galactic cosmic rays through the induced average density gradient, the information encompassed in the angular distributions in the TeV-PeV energy range appear today as a promising tool to infer some properties of the local magnetic field environments. At the highest energies, the extragalactic origin of the particles has been recently determined observationally. While no discrete source of ultrahigh-energy cosmic rays has been identified so far, the noose is tightening around nearby extragalactic objects, and some prospects are discussed.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10303 - Particles and field physics

Result continuities

  • Project

  • Continuities

Others

  • Publication year

    2019

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Astroparticle Physics

  • ISSN

    0927-6505

  • e-ISSN

  • Volume of the periodical

    104

  • Issue of the periodical within the volume

    Jan

  • Country of publishing house

    NL - THE KINGDOM OF THE NETHERLANDS

  • Number of pages

    29

  • Pages from-to

    13-41

  • UT code for WoS article

    000447479300002

  • EID of the result in the Scopus database

    2-s2.0-85052314751