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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...

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Autores principales: Cecchini, S., Chiarusi, Tommaso, Giacomelli, G., Manzoor, S., Medinaceli, E., Patrizii, L., Togo, V.
Lenguaje:eng
Publicado: 2005
Materias:
Acceso en línea:http://cds.cern.ch/record/900376
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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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