1. Experimental motivation and instruments The Cosmic Ray Energetics And Mass
f t the CREAM cosmic ray balloon mission (CREAM) experiment [1] will investigate very launch is foreseen in Antarctica in December 2004. The experiment is intended to observe spectral 12 15 ARTICLE IN PRESSfeatures from 10 to 10 eV and an elemental abundance distribution that might be related to 016...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.456.9684 2023-05-15T13:58:00+02:00 1. Experimental motivation and instruments The Cosmic Ray Energetics And Mass J. H. Sonea J. Yanga The Pennsylvania State University CiteSeerX Archives 2004 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.456.9684 http://www.atic.umd.edu/pub/cream/pub2004/ipark1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.456.9684 http://www.atic.umd.edu/pub/cream/pub2004/ipark1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://www.atic.umd.edu/pub/cream/pub2004/ipark1.pdf Cosmic ray Silicon detector Charge measurement text 2004 ftciteseerx 2016-01-08T06:15:48Z f t the CREAM cosmic ray balloon mission (CREAM) experiment [1] will investigate very launch is foreseen in Antarctica in December 2004. The experiment is intended to observe spectral 12 15 ARTICLE IN PRESSfeatures from 10 to 10 eV and an elemental abundance distribution that might be related to 0168-9002/ $- see front matter r 2004 Elsevier B.V. All rights reserved. doi:10.1016/j.nima.2004.07.147 Corresponding author. Text Antarc* Antarctica Unknown |
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ftciteseerx |
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English |
topic |
Cosmic ray Silicon detector Charge measurement |
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Cosmic ray Silicon detector Charge measurement J. H. Sonea J. Yanga 1. Experimental motivation and instruments The Cosmic Ray Energetics And Mass |
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Cosmic ray Silicon detector Charge measurement |
description |
f t the CREAM cosmic ray balloon mission (CREAM) experiment [1] will investigate very launch is foreseen in Antarctica in December 2004. The experiment is intended to observe spectral 12 15 ARTICLE IN PRESSfeatures from 10 to 10 eV and an elemental abundance distribution that might be related to 0168-9002/ $- see front matter r 2004 Elsevier B.V. All rights reserved. doi:10.1016/j.nima.2004.07.147 Corresponding author. |
author2 |
The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
J. H. Sonea J. Yanga |
author_facet |
J. H. Sonea J. Yanga |
author_sort |
J. H. Sonea J. Yanga |
title |
1. Experimental motivation and instruments The Cosmic Ray Energetics And Mass |
title_short |
1. Experimental motivation and instruments The Cosmic Ray Energetics And Mass |
title_full |
1. Experimental motivation and instruments The Cosmic Ray Energetics And Mass |
title_fullStr |
1. Experimental motivation and instruments The Cosmic Ray Energetics And Mass |
title_full_unstemmed |
1. Experimental motivation and instruments The Cosmic Ray Energetics And Mass |
title_sort |
1. experimental motivation and instruments the cosmic ray energetics and mass |
publishDate |
2004 |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.456.9684 http://www.atic.umd.edu/pub/cream/pub2004/ipark1.pdf |
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Antarc* Antarctica |
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Antarc* Antarctica |
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http://www.atic.umd.edu/pub/cream/pub2004/ipark1.pdf |
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http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.456.9684 http://www.atic.umd.edu/pub/cream/pub2004/ipark1.pdf |
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Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766265937824055296 |