Primary Cosmic Ray Composition at 10 [to the Power] 15--10 [to the Power] 17ev Studied from Extensive Air Shower Simulations PDF Download
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Author: 張增 Publisher: ISBN: 9781374772250 Category : Languages : en Pages :
Book Description
This dissertation, "Primary Cosmic Ray Composition at 10 [to the Power] 15--10 [to the Power] 17eV Studied From Extensive Air Shower Simulations" by 張增, Tsang, Cheung, was obtained from The University of Hong Kong (Pokfulam, Hong Kong) and is being sold pursuant to Creative Commons: Attribution 3.0 Hong Kong License. The content of this dissertation has not been altered in any way. We have altered the formatting in order to facilitate the ease of printing and reading of the dissertation. All rights not granted by the above license are retained by the author. DOI: 10.5353/th_b3123059 Subjects: Cosmic rays Cosmic ray showers
Author: 張增 Publisher: ISBN: 9781374772250 Category : Languages : en Pages :
Book Description
This dissertation, "Primary Cosmic Ray Composition at 10 [to the Power] 15--10 [to the Power] 17eV Studied From Extensive Air Shower Simulations" by 張增, Tsang, Cheung, was obtained from The University of Hong Kong (Pokfulam, Hong Kong) and is being sold pursuant to Creative Commons: Attribution 3.0 Hong Kong License. The content of this dissertation has not been altered in any way. We have altered the formatting in order to facilitate the ease of printing and reading of the dissertation. All rights not granted by the above license are retained by the author. DOI: 10.5353/th_b3123059 Subjects: Cosmic rays Cosmic ray showers
Author: M. V. S. Rao Publisher: World Scientific ISBN: 9789810228880 Category : Science Languages : en Pages : 372
Book Description
Ultrahigh energy cosmic rays carry information about their sources and the intervening medium apart from providing a beam of particles for studying certain features of high energy interactions currently inaccessible at man-made accelerators. They can at present be studied only via the extensive air showers (EAS's) they generate while passing through the Earth's atmosphere, since their fluxes are too low for the experiments of limited capability flown in balloons and satellites. The EAS is generated by a series of interactions of the primary cosmic ray and its progeny with the atmospheric nuclei. The exponential nature of the atmosphere spreads the air showers laterally over several hundreds of meters, thus enabling ground-based arrays of relatively inexpensive detectors to record and study them.This book describes the EAS phenomenology, the detectors and techniques used, and the latest results on the energy spectrum and composition of the primaries of EAS's and the results on high energy interactions obtained from EAS studies. It also describes the new TeV and PeV gamma ray astronomy (which has been developing over the past decade) and the newly emerging neutrino astronomy, which are related to the origin of cosmic rays.This book serves as an introduction as well as a reference for researchers in the field.
Author: Publisher: ISBN: Category : Power resources Languages : en Pages : 872
Book Description
Semiannual, with semiannual and annual indexes. References to all scientific and technical literature coming from DOE, its laboratories, energy centers, and contractors. Includes all works deriving from DOE, other related government-sponsored information, and foreign nonnuclear information. Arranged under 39 categories, e.g., Biomedical sciences, basic studies; Biomedical sciences, applied studies; Health and safety; and Fusion energy. Entry gives bibliographical information and abstract. Corporate, author, subject, report number indexes.
Author: Benjamin S. Flaggs Publisher: ISBN: Category : Languages : en Pages : 0
Book Description
Extensive cosmic ray research has been performed over the course of the last century, yet the origin of the highest energy cosmic rays remains unknown. One way progress is made towards determining the origin of these ultra-high energy charged particles is through precise measurements of their mass composition. However, the highest energy cosmic rays must be detected indirectly via cosmic ray air showers. Therefore the mass of the primary cosmic ray must be derived from information of air shower observables sensitive to the primary particle mass. Specifically, these mass sensitive observables include the depth of shower maximum, and parameters related to the relative size of the muonic component of the air shower. In this thesis, CORSIKA simulations of cosmic ray air showers are used to study the separation power between proton and iron primary cosmic rays, based on combined knowledge of various mass sensitive observables. Specifically, the energy and zenith dependence of observables are investigated in relation to their impact on the proton-iron separation power. For the IceCube Neutrino Observatory, the difference in separation power between high energy penetrating muons and low energy surface muons is investigated. Additionally, the effect of low energy surface muons on proton-iron separation power was studied for the Pierre Auger Observatory and compared to the low energy surface muon separation power obtained from IceCube.
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Author: Tsang Cheung
Author: M. V. S. Rao
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Author: Benjamin S. Flaggs
Author: Bei Cai
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