Observations of the Ultra-Heavy Galactic Cosmic-Ray Abundances (30 ≤ Z ≤ 40) with TIGER
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....
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Tata Institute of Fundamental Research
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ftcaltechauth:oai:authors.library.caltech.edu:49091 2023-05-15T13:55:33+02:00 Observations of the Ultra-Heavy Galactic Cosmic-Ray Abundances (30 ≤ Z ≤ 40) with TIGER Geier, S. Rauch, B. F. Barbier, L. M. Binns, W. R. Cummings, J. R. de Nolfo, G. A. Israel, M. H. Link, J. T. Mewaldt, R. A. Mitchell, J. W. Schindler, S. M. Scott, L. M. Stone, E. C. Streitmatter, R. E. Waddington, C. J. 2005 application/pdf https://authors.library.caltech.edu/49091/ https://authors.library.caltech.edu/49091/1/Stone_2005p93.pdf https://resolver.caltech.edu/CaltechAUTHORS:20140902-091332874 unknown Tata Institute of Fundamental Research https://authors.library.caltech.edu/49091/1/Stone_2005p93.pdf 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 <https://resolver.caltech.edu/CaltechAUTHORS:20140902-091332874> Book Section PeerReviewed 2005 ftcaltechauth 2020-04-26T16:46:44Z 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. Book Part Antarc* Antarctica Caltech Authors (California Institute of Technology) |
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Caltech Authors (California Institute of Technology) |
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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. |
format |
Book Part |
author |
Geier, S. Rauch, B. F. Barbier, L. M. Binns, W. R. Cummings, J. R. de Nolfo, G. A. Israel, M. H. Link, J. T. Mewaldt, R. A. Mitchell, J. W. Schindler, S. M. Scott, L. M. Stone, E. C. Streitmatter, R. E. Waddington, C. J. |
spellingShingle |
Geier, S. Rauch, B. F. Barbier, L. M. Binns, W. R. Cummings, J. R. de Nolfo, G. A. Israel, M. H. Link, J. T. Mewaldt, R. A. Mitchell, J. W. Schindler, S. M. Scott, L. M. Stone, E. C. Streitmatter, R. E. Waddington, C. J. Observations of the Ultra-Heavy Galactic Cosmic-Ray Abundances (30 ≤ Z ≤ 40) with TIGER |
author_facet |
Geier, S. Rauch, B. F. Barbier, L. M. Binns, W. R. Cummings, J. R. de Nolfo, G. A. Israel, M. H. Link, J. T. Mewaldt, R. A. Mitchell, J. W. Schindler, S. M. Scott, L. M. Stone, E. C. Streitmatter, R. E. Waddington, C. J. |
author_sort |
Geier, S. |
title |
Observations of the Ultra-Heavy Galactic Cosmic-Ray Abundances (30 ≤ Z ≤ 40) with TIGER |
title_short |
Observations of the Ultra-Heavy Galactic Cosmic-Ray Abundances (30 ≤ Z ≤ 40) with TIGER |
title_full |
Observations of the Ultra-Heavy Galactic Cosmic-Ray Abundances (30 ≤ Z ≤ 40) with TIGER |
title_fullStr |
Observations of the Ultra-Heavy Galactic Cosmic-Ray Abundances (30 ≤ Z ≤ 40) with TIGER |
title_full_unstemmed |
Observations of the Ultra-Heavy Galactic Cosmic-Ray Abundances (30 ≤ Z ≤ 40) with TIGER |
title_sort |
observations of the ultra-heavy galactic cosmic-ray abundances (30 ≤ z ≤ 40) with tiger |
publisher |
Tata Institute of Fundamental Research |
publishDate |
2005 |
url |
https://authors.library.caltech.edu/49091/ https://authors.library.caltech.edu/49091/1/Stone_2005p93.pdf https://resolver.caltech.edu/CaltechAUTHORS:20140902-091332874 |
genre |
Antarc* Antarctica |
genre_facet |
Antarc* Antarctica |
op_relation |
https://authors.library.caltech.edu/49091/1/Stone_2005p93.pdf 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 <https://resolver.caltech.edu/CaltechAUTHORS:20140902-091332874> |
_version_ |
1766262261496676352 |