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Composition of Cosmic Rays with the Energy more than 4x10^{19} eV
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Search Sources of Cosmic Rays Ultrahigh Energy
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Clusters in Very High Energy Cosmic Rays
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Analysis of the Arrival Directions of Ultrahigh Energy Cosmic Rays
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Search for Sources of Ultrahigh Energy Cosmic Rays
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Galactic origin of ultrahigh energy cosmic rays
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Composition of Cosmic Rays with the Energy more than 4x10^{19} eV
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Search Sources of Cosmic Rays Ultrahigh Energy
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Clusters in Very High Energy Cosmic Rays
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Galactic origin of ultrahigh energy cosmic rays
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Analysis of the Arrival Directions of Ultrahigh Energy Cosmic Rays
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Search for Sources of Ultrahigh Energy Cosmic Rays
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The Determination of the Equator-Point for Observing Star Declinations
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Physical mechanism of strong negative storm effects in the daytime ionospheric F...
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A self-consistent estimate of O + , N 2 -rate coefficient and total EUV flux wit...
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Self-consistent modelling of the daytime electron density profile in the ionosph...
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Equinoctial transitions in the ionosphere and thermosphere
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Geomagnetic storm effects at F1-layer heights from incoherent scatter observatio...
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Self-consistent modelling of the daytime electron density profile in the ionosph...
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Self-consistent modelling of the daytime electron density profile in the ionosph...
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FOS Physical sciences
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[SDU.OCEAN]Sciences of the Universe [physics]/Ocean
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Verlagsveröffentlichung
article
EISCAT
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Astrophysics - High Energy Astrophysical Phenomena
High Energy Astrophysical Phenomena astro-ph.HE
QC1-999
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