Published June 30, 1981
| Version v1
Journal article
Gamma-rays above 100 GeV
Creators
- 1. Durham Univ. (UK)
- 2. Royal Greenwich Observatory, Hailsham (UK)
Description
The Cherenkov light technique for the ground -based detection of ultra-high energy γ-rays is described and some of the most significant measurements are reported. Improvements in experiments leading to increases in sensitivity are outlined and the aims of future work are discussed. (author)
Additional details
Publishing Information
- Journal Title
- Philos. Trans. R. Soc. London, Ser. A
- Journal Volume
- 301
- Journal Issue
- 1462
- Series
- Philos. Trans. R. Soc. London, Ser. A.
- Journal Page Range
- 615-628
- ISSN
- 0080-4614
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 12626162
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CHERENKOV RADIATION; COSMIC GAMMA SOURCES; COSMIC RADIATION; GAMMA ASTRONOMY; GAMMA DETECTION; GAMMA RADIATION; GEV RANGE 100-1000; PHOTONS; SENSITIVITY
- Descriptors DEC
- ASTRONOMY; COSMIC RAY SOURCES; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; ENERGY RANGE; GEV RANGE; IONIZING RADIATIONS; MASSLESS PARTICLES; RADIATION DETECTION; RADIATIONS
Optional Information
- Notes
- Gamma-ray astronomy: a discussion arranged by the British National Committee on Space Research under the leadership of Sir Harrie Massey, F.R.S., A.W. Wolfendale, F.R.S., and R.D. Wills.