Please use this identifier to cite or link to this item: http://hdl.handle.net/10603/69290
Title: Studies on some important properties of UHE air showers
Researcher: Saikia, Julie
Guide(s): Datta, Pranayee
Keywords: Air
Electron
Microprocessor
Parameter
Photomultiplier
Photon
Plastic
Pre-amplifier
University: Gauhati University
Completed Date: 31/12/2003
Abstract: The title of the thesis is quotStudies on some important properties of UHE air showersquot.The thesis comprises of seven chapters. Abstracts of different chapters are given below. Chapter 1: Introduction In the first chapter important characteristics of primary cosmic rays (CR) such as origin, energy spectra and mass composition, development of extensive air shower (EAS) along with GZK cut off, LPM shower, development of pre-shower in the magnetosphere are given. Theoretical background of longitudinal development and lateral distribution of electron- photon cascade are described in detail in this chapter. Chapter 2: Studies on Lateral Distribution of the Electron Component of EAS and Characteristics of Age Parameter [ A review ] Theoretical as well as experimental investigation on lateral distribution of electron component of EAS with primary energy (Ep) in the range ~ 1015 eV -~ 1020 eV made by different workers are reviewed in this chapter. This chapter also includes a review on different important properties of age parameter (s). A brief note on the present work alongwith its justification are also presented. The present work aims at the following aspects. (i) To make a comparative study of different LDFs on the basis of age parameter (a) for Ep lt~1017 eV and also (b) for Epgt~1019eV. (ii) To study the following characteristics of age parameter for giant air showers with Ep gt~1019 eV (a) Variation of s with zenith angle (0) for small bins of Nc (b) Variation of s with No for different small bins of 0. (c) Variation of s with Ep for different small bins of 0. (d) Variation of s with atmospheric depth beyond shower maximum for small bins of No(iii) Identification of the primary particle for energy in the range ~1015- ~1016eV and gt~1019eV using Fenyves model and modified Fenyves model respectively For the above studies, data of the Gauhati University Air Shower Array (GUASA) and the Giant Air Shower Laboratories viz. Yakutsk, Russia and Volcano Ranch, USA are used. Chapter 3: EAS Detection System The existing GUASA is...
Pagination: 
URI: http://hdl.handle.net/10603/69290
Appears in Departments:Department of Physics

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01_title page.pdfAttached File19.11 kBAdobe PDFView/Open
02_certificate.pdf33.87 kBAdobe PDFView/Open
03_dedicated.pdf4.45 kBAdobe PDFView/Open
04_abstract.pdf117.72 kBAdobe PDFView/Open
05_preface.pdf33.73 kBAdobe PDFView/Open
06_acknowledgement.pdf81.13 kBAdobe PDFView/Open
07_content.pdf82.78 kBAdobe PDFView/Open
08_chapter 1.pdf1.47 MBAdobe PDFView/Open
09_chapter 2.pdf798.57 kBAdobe PDFView/Open
10_chapter 3.pdf459.18 kBAdobe PDFView/Open
11_chapter 4.pdf347.07 kBAdobe PDFView/Open
12_chapter 5.pdf1.34 MBAdobe PDFView/Open
13_discussion.pdf201.94 kBAdobe PDFView/Open
14_conclusion and future work.pdf52.5 kBAdobe PDFView/Open
15_appendix a.pdf66.03 kBAdobe PDFView/Open
16_appendix b.pdf62.79 kBAdobe PDFView/Open
17_list of publication.pdf31.04 kBAdobe PDFView/Open
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