A gamma-ray spectral logging system including digital playback, with recommendations for a new generation system

1978 ◽  
Author(s):  
Q Bristow ◽  
J G Conaway ◽  
P G Killeen
Keyword(s):  
Gamma Ray ◽  
Generation System ◽  
New Generation

A new generation gamma ray telescope

1994 ◽  
Vol 351 (2-3) ◽  
pp. 493-512 ◽  
Author(s):  
S.P. Ahlen ◽  
U. Becker ◽  
P. Fisher ◽  
Yu. Galaktionov ◽  
J. Goldstein ◽  
...  
Keyword(s):  
Gamma Ray ◽  
New Generation

scholarly journals 6 months of radioxenon detection in western Europe with the SPALAX-New generation system - Part1: Metrological capabilities

2020 ◽  
Vol 225 ◽  
pp. 106442 ◽  
Author(s):  
Sylvain Topin ◽  
Philippe Gross ◽  
Pascal Achim ◽  
Sylvia Generoso ◽  
Antoine Cagniant ◽  
...  
Keyword(s):  
Western Europe ◽  
Generation System ◽  
New Generation ◽  
Radioxenon Detection

Validation of a new generation system for bottom boundary layer beneath solitary wave

2012 ◽  
Vol 59 (1) ◽  
pp. 46-56 ◽  
Author(s):  
Hitoshi Tanaka ◽  
Bambang Winarta ◽  
Suntoyo ◽  
Hiroto Yamaji
Keyword(s):  
Boundary Layer ◽  
Solitary Wave ◽  
Bottom Boundary Layer ◽  
Generation System ◽  
Bottom Boundary ◽  
New Generation

scholarly journals Design of a new-generation seismic-acoustic monitoring information and analytical system

2020 ◽  
Vol 192 ◽  
pp. 04012
Author(s):  
Andrei Gladyr
Keyword(s):  
Information Technologies ◽  
Acoustic Monitoring ◽  
Generation System ◽  
Modern Information ◽  
Technological Platform ◽  
Analytical System ◽  
New Generation ◽  
Monitoring Information

The analysis of the existing approach to the development of an information and analytical system for seismic-acoustic monitoring is carried out. An approach to the development of a new generation system based on modern information technologies is proposed. The advantages of developing a system based on a universal technological platform are considered.

scholarly journals Gamma-ray Bursts

2005 ◽  
Vol 192 ◽  
pp. 459-466
Author(s):  
Alberto J. Castro-Tirado
Keyword(s):  
Gamma Ray ◽  
Massive Stars ◽  
Gamma Ray Bursts ◽  
Compact Objects ◽  
X Ray ◽  
Long Duration ◽  
Multi Wavelength ◽  
New Generation ◽  
Short Grbs

SummarySince their discovery in 1967 Gamma-ray bursts (GRBs) have been puzzling to astrophysicists. With the advent of a new generation of X–ray satellites in the late 90’s, it was possible to carry out deep multi-wavelength observations of the counterparts associated with the long duration GRBs class just within a few hours of occurrence, thanks to the observation of the fading X-ray emission that follows the more energetic gamma-ray photons once the GRB event has ended. The fact that this emission (the afterglow) extends at longer wavelengths, led to the discovery of optical/IR/radio counterparts in 1997-2003, greatly improving our understanding of these sources. The classical, long duration GRBs, have been observed to originate at cosmological distances in a range of redshifts with 0.1685 ≤ z ≤ 4.50 implying energy releases of ~ 1051 ergs. The recent results on GRB 021004 and GRB 030329 confirm that the central engines that power these extraordinary events are due to be collapse of massive stars rather than the merging of compact objects as previously also suggested. Short GRBs still remain a mystery as no counterparts have been detected so far.

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