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CERN Document Server 6 ჩანაწერია ნაპოვნი  ძიებას დასჭირდა 1.03 წამი. 
1.
The Cosmic Ray Energetics and Mass (CREAM) timing charge detector / 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 et al.
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. [...]
2009 - 12 p. - Published in : Nucl. Instrum. Methods Phys. Res., A 602 (2009) 525-536
2.
Elemental Spectra from the CREAM-I Flight / Ahn, Hoseok ; 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 et al.
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. [...]
2007 - 4 p. - Published in : : 2, pp. 63-66 Fulltext: PDF; External link: INDICO
In : 30th International Cosmic Ray Conference, Merida, Mexico, 3 - 11 Jul 2007, pp.63-66
3.
Measurements of High-Energy Heavy Nuclei with the CREAM-I TRD / Wakely, Scott P (Chicago U.) ; Ahn, H S (Maryland U.) ; Allison, P S (Ohio State U.) ; Bagliesi, M G (U. Siena (main) ; INFN, Siena) ; Beatty, J J (Ohio State U.) ; Bigongiari, G (U. Siena (main) ; INFN, Siena) ; Boyle, P J (Chicago U., EFI) ; Brandt, T J (Ohio State U.) ; Childers, J T (Minnesota U.) ; Conklin, N B (Penn State U.) et al.
The balloon-borne cosmic-ray experiment CREAM-I (Cosmic-Ray Energetics And Mass) completed a successful 42-day flight during the 2004-2005 NASA\/NSF\/NSBF Antarctic expedition. CREAM-I combines an imaging calorimeter with charge detectors and a precision transition radiation detector (TRD). [...]
2007 - 4 p. - Published in : : 2, pp. 187-190 Fulltext: PDF; External link: INDICO
In : 30th International Cosmic Ray Conference, Merida, Mexico, 3 - 11 Jul 2007, pp.187-190
4.
CREAM for high energy composition measurements / Seo, E S ; Ahn, H S ; Allison, P S ; Beatty, J J ; Choi, M J ; Conklin, N B ; Coutu, S ; DuVernois, M A ; Ganel, O ; Kim, K C et al.
Ground-based indirect measurements have shown that the cosmic-ray allparticle spectrum extends many orders of magnitude beyond the energy thought possible for supernova acceleration. Our balloon-borne Cosmic Ray Energetics And Mass (CREAM) experiment is capable of extending direct measurements of cosmic-rays to the supernova energy scale of 1015 eV in a series of Ultra Long Duration Balloon (ULDB) flights. [...]
2003 - 4 p. - Published in : , pp. 2101-2104 Fulltext: PDF; External link: C03-07-31
In : 28th International Cosmic Ray Conferences, v.1-7, Tsukuba, Japan, 31 Jul - 7 Aug 2003, pp.2101-2104
5.
Elemental Spectra from the CREAM-I Flight / Ahn, H.S. (Maryland U.) ; Allison, P.S. (Ohio State U.) ; Bagliesi, M.G. (Siena U. ; INFN, Siena) ; Beatty, J.J. ; Bigongiari, G. (Siena U. ; INFN, Siena) ; Boyle, P. ; Childers, J.T. ; Conklin, N.B. ; Coutu, S. ; DuVernois, M.A. (Minnesota U.) et al.
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. [...]
arXiv:1003.4983.- 2010 - 12 p. - Published in : : 2, pp. 33-36 External link: Preprint
In : 30th International Cosmic Ray Conference, Merida, Mexico, 3 - 11 Jul 2007, pp.33-36
6.
Studies of Signal Waveforms From the Water-Cherenkov Detectors of the Pierre Auger Observatory / Allison, P S
2005 Published version: PDF;
In : 29th International Cosmic Ray Conference, Pune, India, 3 - 10 Aug 2005, pp.357 (v.7)

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