Geier, S. and Rauch, B. F. and Barbier, L. M. and Binns, W. R. and Cummings, J. R. and de Nolfo, G. A. and Israel, M. H. and Link, J. T. and Mewaldt, R. A. and Mitchell, J. W. and Schindler, S. M. and Scott, L. M. and Stone, E. C. and Streitmatter, R. E. and Waddington, C. J.
(2005)
Observations of the Ultra-Heavy Galactic Cosmic-Ray Abundances (30 ≤ Z ≤ 40) with TIGER.
In:
29th International Cosmic Ray Conference.
Vol.3.
Tata Institute of Fundamental Research
, Mumbai, India, pp. 93-96.
https://resolver.caltech.edu/CaltechAUTHORS:20140902-091332874
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Abstract
Observations of Ultra-Heavy galactic cosmic rays (GCR) help to distinguish the possible origins of GCRs.
The Trans-Iron Galactic Element Recorder (TIGER) measures the charge (Z) and energy of GCRs using a
combination of scintillation counters, Cherenkov counters, and a scintillating fiber hodoscope. TIGER has
accumulated data on two successful flights from McMurdo, Antarctica: the first launched in December of
2001 with a total flight duration of 31.8 days and the second in December of 2003 with a total flight duration
of 18 days. We present a preliminary analysis of the combined data from both flights for Ultra-Heavy GCRs.
| Item Type: | Book Section |
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| Additional Information: | © 2005 Tata Institute of Fundamental Research.
This research was supported by the National Aeronautics and Space Administration under grant NNG05WC04G.
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| Group: | Space Radiation Laboratory |
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| Funders: | | Funding Agency | Grant Number |
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| NASA | NNG05WC04G |
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| Other Numbering System: | | Other Numbering System Name | Other Numbering System ID |
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| Space Radiation Laboratory | 2005-29 |
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| Record Number: | CaltechAUTHORS:20140902-091332874 |
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| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20140902-091332874 |
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| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. |
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| ID Code: | 49091 |
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| Collection: | CaltechAUTHORS |
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| Deposited By: |
Tony Diaz
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| Deposited On: | 03 Sep 2014 14:25 |
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| Last Modified: | 09 Mar 2020 13:19 |
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