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Cosmic ray abundance measurements with the CAKE balloon experiment
We present the results from the CAKE (Cosmic Abundance below Knee Energy) balloon experiment which uses nuclear track detectors. The final experiment goal is the determination of the charge spectrum of CR nuclei with Z $>$ 30 in the primary cosmic radiation. The detector, which has a geometric ac...
Autores principales: | , , , , , , |
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Lenguaje: | eng |
Publicado: |
2005
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Materias: | |
Acceso en línea: | http://cds.cern.ch/record/900376 |
_version_ | 1780908689377460224 |
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author | Cecchini, S. Chiarusi, Tommaso Giacomelli, G. Manzoor, S. Medinaceli, E. Patrizii, L. Togo, V. |
author_facet | Cecchini, S. Chiarusi, Tommaso Giacomelli, G. Manzoor, S. Medinaceli, E. Patrizii, L. Togo, V. |
author_sort | Cecchini, S. |
collection | CERN |
description | We present the results from the CAKE (Cosmic Abundance below Knee Energy) balloon experiment which uses nuclear track detectors. The final experiment goal is the determination of the charge spectrum of CR nuclei with Z $>$ 30 in the primary cosmic radiation. The detector, which has a geometric acceptance of $\sim$ 1.7 m$^2$sr, was exposed in a trans-mediterranean stratospheric balloon flight. Calibrations of the detectors used (CR39 and Lexan), scanning strategies and algorithms for tracking particles in an automatic mode are presented. The present status of the results is discussed |
id | cern-900376 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2005 |
record_format | invenio |
spelling | cern-9003762019-09-30T06:29:59Zhttp://cds.cern.ch/record/900376engCecchini, S.Chiarusi, TommasoGiacomelli, G.Manzoor, S.Medinaceli, E.Patrizii, L.Togo, V.Cosmic ray abundance measurements with the CAKE balloon experimentAstrophysics and AstronomyWe present the results from the CAKE (Cosmic Abundance below Knee Energy) balloon experiment which uses nuclear track detectors. The final experiment goal is the determination of the charge spectrum of CR nuclei with Z $>$ 30 in the primary cosmic radiation. The detector, which has a geometric acceptance of $\sim$ 1.7 m$^2$sr, was exposed in a trans-mediterranean stratospheric balloon flight. Calibrations of the detectors used (CR39 and Lexan), scanning strategies and algorithms for tracking particles in an automatic mode are presented. The present status of the results is discussedWe present the results from the CAKE (Cosmic Abundance below Knee Energy) balloon experiment which uses nuclear track detectors. The final experiment goal is the determination of the charge spectrum of CR nuclei with Z > 30 in the primary cosmic radiation. The detector, which has a geometric acceptance of \~ 1.7 m2 sr, was exposed in a trans-mediterranean stratospheric balloon flight. Calibrations of the detectors used (CR39 and Lexan), scanning strategies and algorithms for tracking particles in an automatic mode are presented. The present status of the results is discussedastro-ph/0510717oai:cds.cern.ch:9003762005-10-25 |
spellingShingle | Astrophysics and Astronomy Cecchini, S. Chiarusi, Tommaso Giacomelli, G. Manzoor, S. Medinaceli, E. Patrizii, L. Togo, V. Cosmic ray abundance measurements with the CAKE balloon experiment |
title | Cosmic ray abundance measurements with the CAKE balloon experiment |
title_full | Cosmic ray abundance measurements with the CAKE balloon experiment |
title_fullStr | Cosmic ray abundance measurements with the CAKE balloon experiment |
title_full_unstemmed | Cosmic ray abundance measurements with the CAKE balloon experiment |
title_short | Cosmic ray abundance measurements with the CAKE balloon experiment |
title_sort | cosmic ray abundance measurements with the cake balloon experiment |
topic | Astrophysics and Astronomy |
url | http://cds.cern.ch/record/900376 |
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