Author: D. C. Prosser
Publisher:
ISBN:
Category :
Languages : en
Pages : 179
Book Description
A Search for Gamma-ray Emission at Energies Greater Than 1014eV from Cygnus X-3 and Eight Other Candidate Sources
A Search for Gamma-ray Emission at Energies Greater Than 10"1"4eV from Cygnus X-3 and Eight Other Candidate Sources
A Search for Very High Energy Gamma Ray Emission from Cygnus X-3
Author: Andrew Harold Szentgyorgyi
Publisher:
ISBN:
Category :
Languages : en
Pages : 456
Book Description
Publisher:
ISBN:
Category :
Languages : en
Pages : 456
Book Description
Gamma Ray Astronomy from 1011 to 1014 EV Using the Atmospheric Cerenkov Technique
Author: N. A. Porter
Publisher:
ISBN:
Category : Cherenkov radiation
Languages : en
Pages : 110
Book Description
The atmospheric Cerenkov technique has been widely used over the past two decades to search for point sources of 1011 to 1014 eV gamma rays. In this technique the gamma rays are detected by the Cerenkov light emission from the small air showers that they create in the atmosphere. The basic principles underlying the technique are reviewed with particular reference to the experiments performed to date, (September 1977). The production and absorption processes that pertain to this energy region are discussed. There is strong evidence for the detection of 10^12 eV gamma rays from NP0532, Centaurus A and Cygnus X-3. Models for these, and other sources for which upper limits have been derived, are outlined. There appears to be no other technique that can compete with the atmospheric Cerenkov technique in this energy range. The methods by which the present flux sensitivity can be reduced by factors of 10 - 100 are discussed; it is also possible to extend observations into the previously unexplored 10 - 100 Gev energy range.
Publisher:
ISBN:
Category : Cherenkov radiation
Languages : en
Pages : 110
Book Description
The atmospheric Cerenkov technique has been widely used over the past two decades to search for point sources of 1011 to 1014 eV gamma rays. In this technique the gamma rays are detected by the Cerenkov light emission from the small air showers that they create in the atmosphere. The basic principles underlying the technique are reviewed with particular reference to the experiments performed to date, (September 1977). The production and absorption processes that pertain to this energy region are discussed. There is strong evidence for the detection of 10^12 eV gamma rays from NP0532, Centaurus A and Cygnus X-3. Models for these, and other sources for which upper limits have been derived, are outlined. There appears to be no other technique that can compete with the atmospheric Cerenkov technique in this energy range. The methods by which the present flux sensitivity can be reduced by factors of 10 - 100 are discussed; it is also possible to extend observations into the previously unexplored 10 - 100 Gev energy range.
Index to Theses with Abstracts Accepted for Higher Degrees by the Universities of Great Britain and Ireland and the Council for National Academic Awards
Author:
Publisher:
ISBN:
Category : Dissertations, Academic
Languages : en
Pages : 1112
Book Description
Theses on any subject submitted by the academic libraries in the UK and Ireland.
Publisher:
ISBN:
Category : Dissertations, Academic
Languages : en
Pages : 1112
Book Description
Theses on any subject submitted by the academic libraries in the UK and Ireland.
A Search for Very High Energy Gamma Rays from Cygnus X-3
Author: John R. Jennings
Publisher:
ISBN:
Category : Cygnus X-3
Languages : en
Pages : 508
Book Description
Publisher:
ISBN:
Category : Cygnus X-3
Languages : en
Pages : 508
Book Description
A Search for Celestial Sources of Gamma Rays of Energy Greater Than 100 MEV
Author: David Russell Hearn
Publisher:
ISBN:
Category : Cosmic rays
Languages : en
Pages : 158
Book Description
A gamma-ray detector consisting of scintillation counters and a spark chamber to convert gamma rays to electron-positron pairs was flown with a balloon to an altitude of 125,000 feet for 7 hours on 28 May 1966. The photon spectrum at 4 g cm-2 atmospheric depth is reported. The angular resolution of the detector and method of determining statistical upper limits of fluxes are thoroughly discussed.
Publisher:
ISBN:
Category : Cosmic rays
Languages : en
Pages : 158
Book Description
A gamma-ray detector consisting of scintillation counters and a spark chamber to convert gamma rays to electron-positron pairs was flown with a balloon to an altitude of 125,000 feet for 7 hours on 28 May 1966. The photon spectrum at 4 g cm-2 atmospheric depth is reported. The angular resolution of the detector and method of determining statistical upper limits of fluxes are thoroughly discussed.
Gamma-ray Emission Above 10sup(15)eV from Cygnus X-3 and Other Galactic Sources
A Search for Point Sources of Ultra-high Energy Gamma Rays with an Emphasis on the Binary System Cygnus X-3
Author: Hans Albert Krimm
Publisher:
ISBN:
Category : Astrophysics
Languages : en
Pages : 434
Book Description
Publisher:
ISBN:
Category : Astrophysics
Languages : en
Pages : 434
Book Description