IST/IDA (Innovative Science and Technology/Institute for Defense Analyses) Gamma-Ray Laser Workshop, 21-22 May 1985.

1985 ◽  
Author(s):  
Bohdan Balko ◽  
Leslie Cohen ◽  
Francis X. Hartmann
Keyword(s):  
Gamma Ray ◽  
Science And Technology ◽  
Technology Institute

scholarly journals High brightness gamma-ray production at Fermilab Accelerator Science and Technology (FAST) facility

2017 ◽  
Author(s):  
D. Mihalcea ◽  
B. Jacobson ◽  
A. Murokh ◽  
P. Piot ◽  
J. Ruan
Keyword(s):  
Gamma Ray ◽  
Science And Technology ◽  
High Brightness

scholarly journals Harnessing science for business

2013 ◽  
Vol 9 (1) ◽  
Author(s):  
Malcolm Menzies
Keyword(s):  
New Zealand ◽  
Advisory Committee ◽  
Science And Technology ◽  
Working Party ◽  
Task Group ◽  
Advanced Technology ◽  
High Tech ◽  
Long Line ◽  
The Creation ◽  
Technology Institute

The New Zealand government has announced the creation of a new Advanced Technology Institute – since renamed Callaghan Innovation after the late Sir Paul Callaghan – to be launched in 2013. Callaghan Innovation’s purpose will be ‘to help get New Zealand’s most innovative ideas out of the lab and into the marketplace more quickly and provide a high-tech HQ for innovative New Zealand business’.1 This development is the latest in a long line of attempts to use research, science and technology to boost the country’s economy (Palmer and Miller, 1984; Ministerial Working Party, 1986; Science and Technology Advisory Committee, 1988; Ministerial Task Group, 1991; Ministry of Research, Science and Technology, 2006, 2007). 

On the possible gamma-ray source in Cygnus

1967 ◽  
Vol 31 ◽  
pp. 469-471
Author(s):  
J. G. Duthie ◽  
M. P. Savedoff ◽  
R. Cobb
Keyword(s):  
Gamma Rays ◽  
Gamma Ray ◽  
Right Ascension

A source of gamma rays has been found at right ascension 20h15m, declination +35°, with an uncertainty of 6° in each coordinate. Its flux is (1·5 ± 0·8) x 10-4photons cm-2sec-1at 100 MeV. Possible identifications are reviewed, but no conclusion is reached. The mechanism producing the radiation is also uncertain.

Laboratory Simulation of Lunar Luminescence

1962 ◽  
Vol 14 ◽  
pp. 441-444 ◽  
Author(s):  
J. E. Geake ◽  
H. Lipson ◽  
M. D. Lumb
Keyword(s):  
Science And Technology ◽  
Laboratory Simulation ◽  
The Moon ◽  
Physics Department ◽  
Luminescent Spectrum

Work has recently begun in the Physics Department of the Manchester College of Science and Technology on an attempt to simulate lunar luminescence in the laboratory. This programme is running parallel with that of our colleagues in the Manchester University Astronomy Department, who are making observations of the luminescent spectrum of the Moon itself. Our instruments are as yet only partly completed, but we will describe briefly what they are to consist of, in the hope that we may benefit from the comments of others in the same field, and arrange to co-ordinate our work with theirs.

Solar Flare Energetic Neutral Emission Measurements in the Project Coronas-I

1994 ◽  
Vol 144 ◽  
pp. 635-639
Author(s):  
J. Baláž ◽  
A. V. Dmitriev ◽  
M. A. Kovalevskaya ◽  
K. Kudela ◽  
S. N. Kuznetsov ◽  
...  
Keyword(s):  
Solar Flare ◽  
Energy Range ◽  
Gamma Rays ◽  
Pulse Shape ◽  
Gamma Ray ◽  
Pulse Shape Discrimination ◽  
Shape Discrimination ◽  
Solar Neutron ◽  
Low Altitude

AbstractThe experiment SONG (SOlar Neutron and Gamma rays) for the low altitude satellite CORONAS-I is described. The instrument is capable to provide gamma-ray line and continuum detection in the energy range 0.1 – 100 MeV as well as detection of neutrons with energies above 30 MeV. As a by-product, the electrons in the range 11 – 108 MeV will be measured too. The pulse shape discrimination technique (PSD) is used.

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