Published 2001
| Published
Book Section - Chapter
Open
The Energetic Trans-Iron Composition Experiment (ENTICE) on the Heavy Nuclei Explorer (HNX) Mission
- Creators
-
Israel, M. H.
- Adams, J. H., Jr.
- Barbier, L. M.
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Binns, W. R.
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Christian, E. R.
- Craig, N.
-
Cummings, A. C.
- Cummings, J. R.
- Doke, T.
- Hasebe, N.
- Hayashi, T.
- Lee, D.
-
Leske, R. A.
- Mark, D.
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Mewaldt, R. A.
- Mitchell, J. W.
- Ogura, K.
- Schindler, S. M.
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Stone, E. C.
- Tarl, G.
- Tawara, H.
- Waddington, C. J.
- Westphal, A .J.
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Wiedenbeck, M. E.
- Yasuda, N.
- Others:
- Simon, M.
- Lorenz, E.
- Pohl, M.
Abstract
The HNX mission is composed of the ENTICE and ECCO experiments. The experimental goal of ENTICE is to measure with high precision the elemental abundances of all nuclei with 10≤Z≤82. This will enable us to determine if the injection mechanism for the cosmic ray accelerator is controlled by FIP or Volatility and to study the mix of nucleosynthetic processes that contribute to the galactic cosmic ray source. The ENTICE experiment utilizes the dE/dx-C method of charge determination and consists of silicon dE/dx detectors, Cherenkov detectors with two different refractive indices, and a fiber hodoscope. We will describe the instrument and its performance based on beam tests of a prototype instrument.
Additional Information
© Copernicus GmbH. Provided by the NASA Astrophysics Data System This research was supported in part by the National Aeronautics and Space Administration under grant NAG5- I 0802 and by the McDonnell Center for the Space Sciences at Washington University.Attached Files
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Additional details
- Eprint ID
- 55421
- Resolver ID
- CaltechAUTHORS:20150302-133152754
- NASA
- NAG-10802
- Created
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2015-03-04Created from EPrint's datestamp field
- Updated
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2020-03-09Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Other Numbering System Name
- Space Radiation Laboratory
- Other Numbering System Identifier
- 2001-22