[PDF][PDF] Expected acceptance of the KLYPVE/K-EUSO space-based mission for the observation of ultra-high energy cosmic rays

N Sakaki, S Ogio, F Fenu, M Bertaina, Y Takizawa… - 2015 - pos.sissa.it
More than 50 years have passed since the first 1020 eV candidate was registered [1], but the
origin of cosmic rays with energy above 50 EeV is still a mystery. At present, two …

[PDF][PDF] Expected acceptance of the KLYPVE/K-EUSO space-based mission for the observation of ultra-high energy cosmic rays

N Sakaki, S Ogio, F Fenu, M Bertaina, Y Takizawa… - 2015 - pdfs.semanticscholar.org
More than 50 years have passed since the first 1020 eV candidate was registered [1], but the
origin of cosmic rays with energy above 50 EeV is still a mystery. At present, two …

[PDF][PDF] Expected acceptance of the KLYPVE/K-EUSO space-based mission for the observation of ultra-high energy cosmic rays

N Sakaki, S Ogio, F Fenu, M Bertaina, Y Takizawa… - 2015 - s3.cern.ch
More than 50 years have passed since the first 1020 eV candidate was registered [1], but the
origin of cosmic rays with energy above 50 EeV is still a mystery. At present, two …

[引用][C] Expected acceptance of the KLYPVE/K-EUSO space-based mission for the observation of ultra-high energy cosmic rays

N Sakaki, F Fenu, Y Takizawa… - 34th International …, 2015 - ui.adsabs.harvard.edu
Expected acceptance of the KLYPVE/K-EUSO space-based mission for the observation of
ultra-high energy cosmic rays - NASA/ADS Now on home page ads icon ads Enable full ADS view …

[PDF][PDF] Expected acceptance of the KLYPVE/K-EUSO space-based mission for the observation of ultra-high energy cosmic rays

N Sakaki, S Ogio, F Fenu, M Bertaina, Y Takizawa… - 2015 - inspirehep.net
More than 50 years have passed since the first 1020 eV candidate was registered [1], but the
origin of cosmic rays with energy above 50 EeV is still a mystery. At present, two …

[PDF][PDF] Expected acceptance of the KLYPVE/K-EUSO space-based mission for the observation of ultra-high energy cosmic rays

N Sakaki, S Ogio, F Fenu, M Bertaina, Y Takizawa… - 2015 - galprop.stanford.edu
More than 50 years have passed since the first 1020 eV candidate was registered [1], but the
origin of cosmic rays with energy above 50 EeV is still a mystery. At present, two …

[引用][C] Expected acceptance of the KLYPVE/K-EUSO space-based mission for the observation of ultra-high energy cosmic rays

N Sakaki, S Ogio, F Fenu, M Bertaina, Y Takizawa… - Proceedings of …, 2015 - elibrary.ru
Expected acceptance of the KLYPVE/K-EUSO space-based mission for the observation of
ultra-high energy cosmic rays КОРЗИНА ПОИСК НАВИГАТОР ЖУРНАЛЫ КНИГИ ПАТЕНТЫ …

[PDF][PDF] Expected acceptance of the KLYPVE/K-EUSO space-based mission for the observation of ultra-high energy cosmic rays

N Sakaki, S Ogio, F Fenu, M Bertaina, Y Takizawa… - 2015 - researchgate.net
More than 50 years have passed since the first 1020 eV candidate was registered [1], but the
origin of cosmic rays with energy above 50 EeV is still a mystery. At present, two …

[PDF][PDF] Expected acceptance of the KLYPVE/K-EUSO space-based mission for the observation of ultra-high energy cosmic rays

N Sakaki, S Ogio, F Fenu, M Bertaina, Y Takizawa… - 2015 - scholar.archive.org
More than 50 years have passed since the first 1020 eV candidate was registered [1], but the
origin of cosmic rays with energy above 50 EeV is still a mystery. At present, two …