Elemental spectra from the CREAM-I flight

H. S. Ahn; P. S. Allison; M. G. Bagliesi; J. J. Beatty; G. Bigongiari; P. J. Boyle; J. T. Childers; N. B. Conklin; S. Coutu; M. A. Duvernois; O. Ganel; J. H. Han; J. A. Jeon; K. C. Kim; J. K. Lee; M. H. Lee; L. Lutz; P. Maestro; A. Malinine; P. S. Marrocchesi; S. Minnick; S. I. Mognet; S. Nam; S. Nutter; I. H. Park; N. H. Park; E. S. Seo; R. Sina; S. Swordy; S. P. Wakely; J. Wu; J. Yang; Y. S. Yoon; R. Zei; S. Y. Zinn

Elemental spectra from the CREAM-I flight

H. S. Ahn
, P. S. Allison
, M. G. Bagliesi
, J. J. Beatty
, G. Bigongiari
, P. J. Boyle
, J. T. Childers
, N. B. Conklin
, S. Coutu
, M. A. Duvernois
, O. Ganel
, J. H. Han
, J. A. Jeon
, K. C. Kim
, J. K. Lee
, M. H. Lee
, L. Lutz
, P. Maestro
, A. Malinine
, P. S. Marrocchesi

S. Minnick, S. I. Mognet, S. Nam, S. Nutter, I. H. Park, N. H. Park, E. S. Seo, R. Sina, S. Swordy, S. P. Wakely, J. Wu, J. Yang, Y. S. Yoon, R. Zei, S. Y. Zinn

Research output: Contribution to conference › Paper › peer-review

3 Scopus citations

Abstract

The Cosmic Ray Energetics And Mass (CREAM) instrument 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 1015 eV. CREAM had two successful flights on long-duration balloons (LDB) launched from McMurdo Station, Antarctica, in December 2004 and December 2005. CREAM achieves a substantial measurement redundancy by employing multiple detector systems, namely a Timing Charge Detector (TCD), a Silicon Charge Detector (SCD), and a Cherenkov Detector (CD) for particle identification, and a Transition Radiation Detector (TRD) 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.

Original language	English (US)
Pages	63-66
Number of pages	4
State	Published - 2007
Event	30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan, Mexico Duration: Jul 3 2007 → Jul 11 2007

Other

Other	30th International Cosmic Ray Conference, ICRC 2007
Country/Territory	Mexico
City	Merida, Yucatan
Period	7/3/07 → 7/11/07

All Science Journal Classification (ASJC) codes

Nuclear and High Energy Physics

Cite this

Ahn, H. S., Allison, P. S., Bagliesi, M. G., Beatty, J. J., Bigongiari, G., Boyle, P. J., 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., Malinine, A., ... Zinn, S. Y. (2007). Elemental spectra from the CREAM-I flight. 63-66. Paper presented at 30th International Cosmic Ray Conference, ICRC 2007, Merida, Yucatan, Mexico.

@conference{45d37e5dd4344d76a591ae9f4eaeabd7,

title = "Elemental spectra from the CREAM-I flight",

abstract = "The Cosmic Ray Energetics And Mass (CREAM) instrument 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 1015 eV. CREAM had two successful flights on long-duration balloons (LDB) launched from McMurdo Station, Antarctica, in December 2004 and December 2005. CREAM achieves a substantial measurement redundancy by employing multiple detector systems, namely a Timing Charge Detector (TCD), a Silicon Charge Detector (SCD), and a Cherenkov Detector (CD) for particle identification, and a Transition Radiation Detector (TRD) 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.",

author = "Ahn, \{H. S.\} and Allison, \{P. S.\} and Bagliesi, \{M. G.\} and Beatty, \{J. J.\} and G. Bigongiari and Boyle, \{P. J.\} and Childers, \{J. T.\} and Conklin, \{N. B.\} and S. Coutu and Duvernois, \{M. A.\} and O. Ganel and Han, \{J. H.\} and Jeon, \{J. A.\} and Kim, \{K. C.\} and Lee, \{J. K.\} and Lee, \{M. H.\} and L. Lutz and P. Maestro and A. Malinine and Marrocchesi, \{P. S.\} and S. Minnick and \{I. Mognet\}, S. and S. Nam and S. Nutter and Park, \{I. H.\} and Park, \{N. H.\} and Seo, \{E. S.\} and R. Sina and S. Swordy and Wakely, \{S. P.\} and J. Wu and J. Yang and Yoon, \{Y. S.\} and R. Zei and Zinn, \{S. Y.\}",

year = "2007",

language = "English (US)",

pages = "63--66",

note = "30th International Cosmic Ray Conference, ICRC 2007 ; Conference date: 03-07-2007 Through 11-07-2007",

}

Ahn, HS, Allison, PS, Bagliesi, MG, Beatty, JJ, Bigongiari, G, Boyle, PJ, Childers, JT, Conklin, NB, Coutu, S, Duvernois, MA, Ganel, O, Han, JH, Jeon, JA, Kim, KC, Lee, JK, Lee, MH, Lutz, L, Maestro, P, Malinine, A, Marrocchesi, PS, Minnick, S, I. Mognet, S, Nam, S, Nutter, S, Park, IH, Park, NH, Seo, ES, Sina, R, Swordy, S, Wakely, SP, Wu, J, Yang, J, Yoon, YS, Zei, R & Zinn, SY 2007, 'Elemental spectra from the CREAM-I flight', Paper presented at 30th International Cosmic Ray Conference, ICRC 2007, Merida, Yucatan, Mexico, 7/3/07 - 7/11/07 pp. 63-66.

TY - CONF

T1 - Elemental spectra from the CREAM-I flight

AU - Ahn, H. S.

AU - Allison, P. S.

AU - Bagliesi, M. G.

AU - Beatty, J. J.

AU - Bigongiari, G.

AU - Boyle, P. J.

AU - Childers, J. T.

AU - Conklin, N. B.

AU - Coutu, S.

AU - Duvernois, M. A.

AU - Ganel, O.

AU - Han, J. H.

AU - Jeon, J. A.

AU - Kim, K. C.

AU - Lee, J. K.

AU - Lee, M. H.

AU - Lutz, L.

AU - Maestro, P.

AU - Malinine, A.

AU - Marrocchesi, P. S.

AU - Minnick, S.

AU - I. Mognet, S.

AU - Nam, S.

AU - Nutter, S.

AU - Park, I. H.

AU - Park, N. H.

AU - Seo, E. S.

AU - Sina, R.

AU - Swordy, S.

AU - Wakely, S. P.

AU - Wu, J.

AU - Yang, J.

AU - Yoon, Y. S.

AU - Zei, R.

AU - Zinn, S. Y.

PY - 2007

Y1 - 2007

N2 - The Cosmic Ray Energetics And Mass (CREAM) instrument 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 1015 eV. CREAM had two successful flights on long-duration balloons (LDB) launched from McMurdo Station, Antarctica, in December 2004 and December 2005. CREAM achieves a substantial measurement redundancy by employing multiple detector systems, namely a Timing Charge Detector (TCD), a Silicon Charge Detector (SCD), and a Cherenkov Detector (CD) for particle identification, and a Transition Radiation Detector (TRD) 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.

AB - The Cosmic Ray Energetics And Mass (CREAM) instrument 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 1015 eV. CREAM had two successful flights on long-duration balloons (LDB) launched from McMurdo Station, Antarctica, in December 2004 and December 2005. CREAM achieves a substantial measurement redundancy by employing multiple detector systems, namely a Timing Charge Detector (TCD), a Silicon Charge Detector (SCD), and a Cherenkov Detector (CD) for particle identification, and a Transition Radiation Detector (TRD) 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.

UR - https://www.scopus.com/pages/publications/84891253707

UR - https://www.scopus.com/pages/publications/84891253707#tab=citedBy

M3 - Paper

AN - SCOPUS:84891253707

SP - 63

EP - 66

T2 - 30th International Cosmic Ray Conference, ICRC 2007

Y2 - 3 July 2007 through 11 July 2007

ER -

Elemental spectra from the CREAM-I flight

Abstract

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All Science Journal Classification (ASJC) codes

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