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- W4387130862 abstract "Existing small, medium and large arrays for the study of cosmic rays of ultra-high energies are aimed for obtaining information about our galaxy and extragalactic space, namely to search and study astronomical objects that produce the flux of relativistic particles. The drift and interaction of such particles with magnetic fields and shock waves taking place in interstellar space causes the same interest. The shape of the energy spectrum of cosmic rays in the energy range 10^{15}-10^{18} <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mrow><mml:msup><mml:mn>10</mml:mn><mml:mn>15</mml:mn></mml:msup><mml:mo>−</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math> eV, where the knee and the second knee’’ are observed, can be formed as a superposition of the partial spectra of various chemical elements. Verification of galactic models, using recent experimental spectral data, makes it possible to study the nature of the galactic and extragalactic components of cosmic rays. The paper presents the result of the energy spectrum of cosmic rays in the range 10^{16}-10^{18} <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mrow><mml:msup><mml:mn>10</mml:mn><mml:mn>16</mml:mn></mml:msup><mml:mo>−</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math> eV of measurements obtained with the Small Cherenkov array - a part of the Yakutsk array." @default.
- W4387130862 created "2023-09-29" @default.
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- W4387130862 date "2023-09-28" @default.
- W4387130862 modified "2023-10-18" @default.
- W4387130862 title "On irregularities in the cosmic ray spectrum of (10^{16}-10^{18}) eV range" @default.
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- W4387130862 doi "https://doi.org/10.21468/scipostphysproc.13.020" @default.
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