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- W2015721465 abstract "The proton component has been extensively studied at high altitudes on a series of 6 Skyhook balloon flights at various latitudes using the ifmmode check{C}else v{C}fi{}erenkov-scintillation counter technique. The intensity of primary protons has been measured at 4ifmmode^circelsetextdegreefi{}, 41ifmmode^circelsetextdegreefi{}, 53ifmmode^circelsetextdegreefi{}, and 55ifmmode^circelsetextdegreefi{} geomagnetic latitude. The proton differential energy spectrum has been measured directly in the region 250-750 Mev. It is observed that primary alphas and protons have the same form of rigidity spectrum from 1 Bv to 17 Bv. A series of cutoff rigidities are measured in the vicinity of $ensuremath{lambda}=53ifmmode^circelsetextdegreefi{} mathrm{and} 55ifmmode^circelsetextdegreefi{}$. The intensity and composition of fast splash albedo is determined at $ensuremath{lambda}=4ifmmode^circelsetextdegreefi{}, 53ifmmode^circelsetextdegreefi{}, mathrm{and} 55ifmmode^circelsetextdegreefi{}$. Significant time variations are observed between the three high-latitude flights. Differences observed in the intensity and energy spectra of these three flights are discussed and strong restraints are placed on possible modulating mechanisms." @default.
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- W2015721465 date "1959-07-01" @default.
- W2015721465 modified "2023-09-28" @default.
- W2015721465 title "Proton Component of the Primary Cosmic Radiation" @default.
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- W2015721465 doi "https://doi.org/10.1103/physrev.115.194" @default.
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