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  • About
  • The Global ETD Search service is a free service for researchers to find electronic theses and dissertations. This service is provided by the Networked Digital Library of Theses and Dissertations.
    Our metadata is collected from universities around the world. If you manage a university/consortium/country archive and want to be added, details can be found on the NDLTD website.
1

A large detector for cosmic ray abundance and energy measurements

Alsop, C. January 1988 (has links)
No description available.
2

The longitudinal development of extensive air showers at energies above 10sup(17)eV

England, C. D. January 1984 (has links)
No description available.
3

The search for ultra high energy gamma ray emission from Cygnus X-3 and Hercules X-1

Bloomer, Steven David January 1990 (has links)
No description available.
4

Measurements of scintillation and water-Cerenkov detector densities in extensive air showers produced by 10sup(16) - 5x10sup(19) eV cosmic rays

Perrett, J. C. January 1985 (has links)
No description available.
5

The determination of the muon content of EAS from CygnusX-3

Bullock, A. D. January 1988 (has links)
No description available.
6

Mass composition of primary cosmic rays in the energy range 10sup(17)-10sup(18)eV

Sephton, A. J. January 1985 (has links)
No description available.
7

A study of the atmospheric neutrino flavour content using the Soudan 2 detector

Stassinakis, Argyrios January 1997 (has links)
No description available.
8

A study of underground muons in the Soudan II Detector

Kirby-Gallagher, Lucy Mary January 1990 (has links)
No description available.
9

An experimental study of the possible association of deep underground muons with astronomical point sources

Thomson, Mark Andrew January 1991 (has links)
No description available.
10

Extensive air showers

Madani, Jamal Hamzah January 1987 (has links)
A computerised 8-channel data acquisition unit constructed by the Durham University Microprocessor Unit is described and the calibration of this unit is given in chapter 2. A test for the data acquisition unit using a Geiger-Mul1er cosmic ray telescope is described in Chapter 3. In Chapter 4 the main experiment is described. Two plastic scintillation counters each of 0.4 area and 5cm thick in coincidence were used in this experiment to measure the density spectrum of electrons at sea level in the range 20 - 600 electrons per m(^2). The microcomputer data acquisition system is employed to record the scintillator pulse heights. The measured integral density spectrum has been used to calculate the integral size spectrum at sea level. A brief description of the theory of electron-photon cascades and the formation of extensive are showers is give in Chapter 5.A FORTRAN program which uses Monte Carlo method to simulate extensive air showers generated by high energy protons with a given energy is described in Chapter 6. Using the relation between primary energy and average number of electrons arriving at sea level found by Monte Carlo calculation in Chapter 6 an estimate has been made of the integral primary energy spectrum in the range lO(^14)-lQ(^16)eV, and the result is given in Chapter 7.

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