Elemental Spectra from the CREAM-I Flight

The Cosmic Ray Energetics And Mass (CREAM) is a balloon-borne experiment designed to measure the composition and energy spectra of cosmic rays of charge Z = 1 to 26 up to an energy of ~ 10^15 eV. CREAM had two successful flights on long-duration balloons (LDB) launched from Mc- Murdo Station, Antarc...

Full description

Bibliographic Details
Main Authors: Ahn, H.S., Allison, P.S., Bagliesi, M.G., Beatty, J.J., Bigongiari, G., Boyle, P., Childers, J.T., Conklin, N.B., Coutu, S., DuVernois, M.A., Ganel, O., Han, J.H., Jeon, J.A., Kim, K.C., Lee, J.K., Lee, M.H., Lutz, L., Maestro, P., Malinin, A., Marrocchesi, P.S., Minnick, S.A., Mognet, S.I., Nam, S.W., Nutter, S.L., Park, I.H., Park, N.H., Seo, E.S., Sina, R., Swordy, S., Wakely, S., Swordy, S.P., Wakely, S.P., Wu, J., Yang, J., Yoon, Y.S., Zei, R., Zinn, S.Y.
Language:English
Published: 2010
Subjects:
Online Access:http://cds.cern.ch/record/1255645
id ftcern:oai:cds.cern.ch:1255645
record_format openpolar
spelling ftcern:oai:cds.cern.ch:1255645 2024-09-15T17:42:22+00:00 Elemental Spectra from the CREAM-I Flight Ahn, H.S. Allison, P.S. Bagliesi, M.G. Beatty, J.J. Bigongiari, G. Boyle, P. Childers, J.T. Conklin, N.B. Coutu, S. DuVernois, M.A. Ganel, O. Han, J.H. Jeon, J.A. Kim, K.C. Lee, J.K. Lee, M.H. Lutz, L. Maestro, P. Malinin, A. Marrocchesi, P.S. Minnick, S.A. Mognet, S.I. Nam, S.W. Nutter, S.L. Park, I.H. Park, N.H. Seo, E.S. Sina, R. Swordy, S. Wakely, S. Swordy, S.P. Wakely, S.P. Wu, J. Yang, J. Yoon, Y.S. Zei, R. Zinn, S.Y. 2010-03-26 http://cds.cern.ch/record/1255645 eng eng http://cds.cern.ch/record/1255645 arXiv:1003.4983 oai:cds.cern.ch:1255645 Astrophysics and Astronomy 2010 ftcern 2024-07-22T14:22:27Z The Cosmic Ray Energetics And Mass (CREAM) is a balloon-borne experiment designed to measure the composition and energy spectra of cosmic rays of charge Z = 1 to 26 up to an energy of ~ 10^15 eV. CREAM had two successful flights on long-duration balloons (LDB) launched from Mc- Murdo Station, Antarctica, in December 2004 and December 2005. CREAM-I achieves a substantial measurement redundancy by employing multiple detector systems, namely a Timing Charge Detector and a Silicon Charge Detector (SCD) for particle identification, and a Transition Radiation Detector and a sampling tungsten/scintillating-fiber ionization calorimeter (CAL) for energy measurement. In this paper, preliminary energy spectra of various elements measured with CAL/SCD during the first 42-day flight are presented. The Cosmic Ray Energetics And Mass (CREAM) is a balloon-borne experiment designed to measure the composition and energy spectra of cosmic rays of charge Z = 1 to 26 up to an energy of ~ 10^15 eV. CREAM had two successful flights on long-duration balloons (LDB) launched from Mc- Murdo Station, Antarctica, in December 2004 and December 2005. CREAM-I achieves a substantial measurement redundancy by employing multiple detector systems, namely a Timing Charge Detector and a Silicon Charge Detector (SCD) for particle identification, and a Transition Radiation Detector and a sampling tungsten/scintillating-fiber ionization calorimeter (CAL) for energy measurement. In this paper, preliminary energy spectra of various elements measured with CAL/SCD during the first 42-day flight are presented. The use of detectors based on plastic scintillator with photomultiplier tubes (PMTs) is common in cosmic-ray experiments to differentiate particle charges. However, in the presence of a calorimeter, the standard method of pulse charge integration over a time longer than a PMT pulse is hampered by abundant albedo particles. The Cosmic Ray Energetics and Mass (CREAM) instrument surmounts this problem by measuring the peak voltage of the PMT pulse ... Other/Unknown Material Antarc* Antarctica CERN Document Server (CDS)
institution Open Polar
collection CERN Document Server (CDS)
op_collection_id ftcern
language English
topic Astrophysics and Astronomy
spellingShingle Astrophysics and Astronomy
Ahn, H.S.
Allison, P.S.
Bagliesi, M.G.
Beatty, J.J.
Bigongiari, G.
Boyle, P.
Childers, J.T.
Conklin, N.B.
Coutu, S.
DuVernois, M.A.
Ganel, O.
Han, J.H.
Jeon, J.A.
Kim, K.C.
Lee, J.K.
Lee, M.H.
Lutz, L.
Maestro, P.
Malinin, A.
Marrocchesi, P.S.
Minnick, S.A.
Mognet, S.I.
Nam, S.W.
Nutter, S.L.
Park, I.H.
Park, N.H.
Seo, E.S.
Sina, R.
Swordy, S.
Wakely, S.
Swordy, S.P.
Wakely, S.P.
Wu, J.
Yang, J.
Yoon, Y.S.
Zei, R.
Zinn, S.Y.
Elemental Spectra from the CREAM-I Flight
topic_facet Astrophysics and Astronomy
description The Cosmic Ray Energetics And Mass (CREAM) is a balloon-borne experiment designed to measure the composition and energy spectra of cosmic rays of charge Z = 1 to 26 up to an energy of ~ 10^15 eV. CREAM had two successful flights on long-duration balloons (LDB) launched from Mc- Murdo Station, Antarctica, in December 2004 and December 2005. CREAM-I achieves a substantial measurement redundancy by employing multiple detector systems, namely a Timing Charge Detector and a Silicon Charge Detector (SCD) for particle identification, and a Transition Radiation Detector and a sampling tungsten/scintillating-fiber ionization calorimeter (CAL) for energy measurement. In this paper, preliminary energy spectra of various elements measured with CAL/SCD during the first 42-day flight are presented. The Cosmic Ray Energetics And Mass (CREAM) is a balloon-borne experiment designed to measure the composition and energy spectra of cosmic rays of charge Z = 1 to 26 up to an energy of ~ 10^15 eV. CREAM had two successful flights on long-duration balloons (LDB) launched from Mc- Murdo Station, Antarctica, in December 2004 and December 2005. CREAM-I achieves a substantial measurement redundancy by employing multiple detector systems, namely a Timing Charge Detector and a Silicon Charge Detector (SCD) for particle identification, and a Transition Radiation Detector and a sampling tungsten/scintillating-fiber ionization calorimeter (CAL) for energy measurement. In this paper, preliminary energy spectra of various elements measured with CAL/SCD during the first 42-day flight are presented. The use of detectors based on plastic scintillator with photomultiplier tubes (PMTs) is common in cosmic-ray experiments to differentiate particle charges. However, in the presence of a calorimeter, the standard method of pulse charge integration over a time longer than a PMT pulse is hampered by abundant albedo particles. The Cosmic Ray Energetics and Mass (CREAM) instrument surmounts this problem by measuring the peak voltage of the PMT pulse ...
author Ahn, H.S.
Allison, P.S.
Bagliesi, M.G.
Beatty, J.J.
Bigongiari, G.
Boyle, P.
Childers, J.T.
Conklin, N.B.
Coutu, S.
DuVernois, M.A.
Ganel, O.
Han, J.H.
Jeon, J.A.
Kim, K.C.
Lee, J.K.
Lee, M.H.
Lutz, L.
Maestro, P.
Malinin, A.
Marrocchesi, P.S.
Minnick, S.A.
Mognet, S.I.
Nam, S.W.
Nutter, S.L.
Park, I.H.
Park, N.H.
Seo, E.S.
Sina, R.
Swordy, S.
Wakely, S.
Swordy, S.P.
Wakely, S.P.
Wu, J.
Yang, J.
Yoon, Y.S.
Zei, R.
Zinn, S.Y.
author_facet Ahn, H.S.
Allison, P.S.
Bagliesi, M.G.
Beatty, J.J.
Bigongiari, G.
Boyle, P.
Childers, J.T.
Conklin, N.B.
Coutu, S.
DuVernois, M.A.
Ganel, O.
Han, J.H.
Jeon, J.A.
Kim, K.C.
Lee, J.K.
Lee, M.H.
Lutz, L.
Maestro, P.
Malinin, A.
Marrocchesi, P.S.
Minnick, S.A.
Mognet, S.I.
Nam, S.W.
Nutter, S.L.
Park, I.H.
Park, N.H.
Seo, E.S.
Sina, R.
Swordy, S.
Wakely, S.
Swordy, S.P.
Wakely, S.P.
Wu, J.
Yang, J.
Yoon, Y.S.
Zei, R.
Zinn, S.Y.
author_sort Ahn, H.S.
title Elemental Spectra from the CREAM-I Flight
title_short Elemental Spectra from the CREAM-I Flight
title_full Elemental Spectra from the CREAM-I Flight
title_fullStr Elemental Spectra from the CREAM-I Flight
title_full_unstemmed Elemental Spectra from the CREAM-I Flight
title_sort elemental spectra from the cream-i flight
publishDate 2010
url http://cds.cern.ch/record/1255645
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_relation http://cds.cern.ch/record/1255645
arXiv:1003.4983
oai:cds.cern.ch:1255645
_version_ 1810488901518753792