scholarly journals HIGH RESOLUTION SPECTROMETER SYSTEM WITH PARTICLE IDENTIFICATION FOR 1- THROUGH 60-MeV HYDROGEN AND HELIUM PARTICLES.

1972 ◽  
Author(s):  
F. E. Bertrand ◽  
W. R. Burrus ◽  
N. W. Hill ◽  
T. A. Love ◽  
R. W. Peelle
Keyword(s):  
High Resolution ◽  
Particle Identification ◽  
High Resolution Spectrometer ◽  
Spectrometer System ◽  
Resolution Spectrometer

Ultra-high resolution spectrometer system for charged particle studies of nuclei

1971 ◽  
Vol 91 (1) ◽  
pp. 61-65 ◽  
Author(s):  
H.G. Blosser ◽  
G.M. Crawley ◽  
R. Deforest ◽  
E. Kashy ◽  
B.H. Wildenthal
Keyword(s):  
Charged Particle ◽  
High Resolution ◽  
High Resolution Spectrometer ◽  
Spectrometer System ◽  
Resolution Spectrometer

Nuclear analysis of the DEMO divertor survey visible high-resolution spectrometer

2021 ◽  
Vol 169 ◽  
pp. 112460
Author(s):  
R. Luís ◽  
Y. Nietiadi ◽  
A. Silva ◽  
B. Gonçalves ◽  
T. Franke ◽  
...  
Keyword(s):  
High Resolution ◽  
Nuclear Analysis ◽  
High Resolution Spectrometer ◽  
Resolution Spectrometer

Low pressure spark chambers — high resolution spectrometer for 1 GeV protons

1967 ◽  
Vol 54 (1) ◽  
pp. 71-76 ◽  
Author(s):  
R.J. Sutter ◽  
G. Bennett ◽  
J. Fischer ◽  
J.L. Friedes ◽  
H. Palevsky ◽  
...  
Keyword(s):  
High Resolution ◽  
Low Pressure ◽  
High Resolution Spectrometer ◽  
Resolution Spectrometer

scholarly journals HERMES – An instrument of the future

2009 ◽  
Vol 5 (S262) ◽  
pp. 448-449 ◽  
Author(s):  
Elizabeth Wylie-de Boer ◽  
Kenneth Freeman
Keyword(s):  
Star Formation ◽  
High Resolution ◽  
Resolving Power ◽  
Individual Stars ◽  
Elemental Abundances ◽  
The Future ◽  
The Galaxy ◽  
History Of ◽  
High Resolution Spectrometer ◽  
Resolution Spectrometer

AbstractHERMES is a new, multi-object high resolution spectrometer for the 3.9m Anglo Australian Telescope, using the existing 2dF positioner. The primary goal of the HERMES survey is to unravel the history of the Galaxy from detailed elemental abundances for about 1.2 million individual stars. The HERMES chemical tagging survey concentrates on the 5000 to 8000 Å window at a resolving power of 30,000 in order to identify dissolved star formation aggregates and ascertain the importance of mergers throughout the history of the Galaxy.

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