25 results on '"Y. Shikaze"'
Search Results
2. Precise Measurements of Hydrogen and Helium Isotopes with BESS-Polar II
- Author
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Kohei Yoshimura, Masaya Hasegawa, Takamasa Yamagami, M. H. Lee, Yasuhiro Makida, Kengo Takeuchi, Jippei Suzuki, M. Sasaki, Y. Shikaze, R. E. Streitmatter, K. Matsumoto, Y. Matsukawa, N. Thakur, Kwangmoo Kim, A. A. Moiseev, T. Kumazawa, A. Itazaki, Sumio Matsuda, Thomas Hams, H. Fuke, R. Shinoda, Kazushi Tanaka, K. Abe, Y. Takasugi, Toshikatsu Yoshida, Mitsuaki Nozaki, John Mitchell, A. Kusumoto, Eun-Suk Seo, Sadakazu Haino, A. Horikoshi, N. Picot-Clemente, J. F. Ormes, Reiko Orito, J. Nishimura, K. Sakai, and Akira Yamamoto
- Subjects
Nuclear physics ,Physics ,Interstellar medium ,Helium-4 ,Deuterium ,Astrophysics::High Energy Astrophysical Phenomena ,Helium-3 ,Cosmic ray ,Spallation ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Nuclear Experiment ,Isotopes of helium ,Galaxy - Abstract
A precise knowledge of cosmic-ray hydrogen and helium isotopes provides important information to better understand Galactic cosmic-ray propagation. Deuteron and helium 3 species are mainly secondary particles created by the spallation of primary proton and helium 4 particles during their propagation in the Galaxy. Secondary-to-primary ratios thus bring direct information on the average amount of material traversed by cosmic rays in the interstellar medium. The Balloon-borne Experiment with Superconducting Spectrometer BESS-Polar II flew over Antarctica for 24.5 days from December 2007 through January 2008, during the 23rd solar cycle minimum. The instrument is made of complementary particle detectors which allow to precisely measure the charge, velocity and rigidity of incident cosmic rays. It can accurately separate and precisely measure cosmic-ray hydrogen and helium isotopes between 0.2 and 1.5 GeV/nucleon. These data, which are the most precise to date, will be reported and their implications will be discussed.
- Published
- 2017
3. BESS-Polar experiment: Progress and future prospects
- Author
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Hideyuki Fuke, A. A. Moiseev, R. Shinoda, A. Kusumoto, Koji Yoshimura, T. Kumazawa, A. Horikoshi, K. Abe, J. Nishimura, Kazuhiro Tanaka, K. Takeuchi, Sadakazu Haino, Y. Makida, R. E. Streitmatter, John Mitchell, Akira Yamamoto, Jun-ichi Suzuki, Y. Shikaze, Y. Matsukawa, Thomas Hams, Mitsuaki Nozaki, K. C. Kim, Jonathan F. Ormes, M. Sasaki, N. Thakur, Eun-Suk Seo, Shinya Matsuda, Takamasa Yamagami, Reiko Orito, Tetsuya Yoshida, Masaya Hasegawa, M. H. Lee, and Kenichi Sakai
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Physics ,Nuclear physics ,Solar minimum ,Atmospheric Science ,Geophysics ,Spectrometer ,Space and Planetary Science ,business.industry ,Aerospace Engineering ,General Earth and Planetary Sciences ,Astronomy and Astrophysics ,Aerospace engineering ,business - Abstract
著者人数: 33名, 資料番号: SA1000089000
- Published
- 2008
4. Search for antihelium: Progress with BESS
- Author
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A. A. Moiseev, Thomas Hams, K. Abe, J. Nishimura, K. C. Kim, Hideyuki Fuke, Eun-Suk Seo, Sadakazu Haino, R. E. Streitmatter, Akira Yamamoto, M. Sasaki, Jonathan F. Ormes, T. Yoshida, John Mitchell, Takamasa Yamagami, S. Orito, Shinya Matsuda, Kazuhiro Tanaka, Mitsuaki Nozaki, M. H. Lee, T. Sanuki, Jun-ichi Suzuki, Y. Shikaze, Koji Yoshimura, and Yasuhiro Makida
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Physics ,Atmospheric Science ,Flight duration ,Geophysics ,Rigidity (electromagnetism) ,Space and Planetary Science ,Antimatter ,Aerospace Engineering ,General Earth and Planetary Sciences ,Astronomy and Astrophysics ,Cosmic ray ,Astrophysics - Abstract
著者人数: 25名, 資料番号: SA1000090000
- Published
- 2008
5. Search for primordial antiparticles with BESS
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Akira Yamamoto, Thomas Hams, Kazuhiro Tanaka, R. Shinoda, M. Sasaki, Koji Yoshimura, Sadakazu Haino, R. E. Streitmatter, Y. Shikaze, J. Nishimura, N. Thakur, Jun-ichi Suzuki, Y. Matsukawa, A. A. Moiseev, Tetsuya Yoshida, Mitsuaki Nozaki, S. Orito, K. Abe, Yasuhiro Makida, Shinya Matsuda, A. Kusumoto, Jonathan F. Ormes, A. Horikoshi, Hideyuki Fuke, Takamasa Yamagami, Masaya Hasegawa, M. H. Lee, T. Sanuki, K. C. Kim, Eun-Suk Seo, Kenichi Sakai, Reiko Orito, and John Mitchell
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Physics ,Atmospheric Science ,Range (particle radiation) ,Antiparticle ,Astrophysics::High Energy Astrophysical Phenomena ,High Energy Physics::Phenomenology ,Astrophysics::Instrumentation and Methods for Astrophysics ,Aerospace Engineering ,Astronomy ,Astronomy and Astrophysics ,Cosmic ray ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Geophysics ,Space and Planetary Science ,Antiproton ,General Earth and Planetary Sciences ,Superconducting spectrometer ,Nuclear Experiment ,Short duration - Abstract
著者人数: 33名, 資料番号: SA1000088000
- Published
- 2008
6. Search for fractionally charged particles in cosmic rays with the BESS spectrometer
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Jun-ichi Suzuki, Sadakazu Haino, Kazuhiro Tanaka, Tetsuya Yoshida, Y. Shikaze, Shinya Matsuda, Yasuhiro Makida, M. Sasaki, A. A. Moiseev, John Mitchell, R. E. Streitmatter, Takamasa Yamagami, Jonathan F. Ormes, S. Orito, Y. Tasaki, K. Abe, Mitsuaki Nozaki, Hideyuki Fuke, Koji Yoshimura, Akira Yamamoto, J. Nishimura, and Eun-Suk Seo
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Physics ,Atmospheric Science ,Spectrometer ,Aerospace Engineering ,Flux ,Astronomy and Astrophysics ,Cosmic ray ,Scintillator ,Charged particle ,Atmosphere ,Nuclear physics ,Geophysics ,Deposition (aerosol physics) ,Space and Planetary Science ,General Earth and Planetary Sciences ,Superconducting spectrometer - Abstract
著者人数: 22名, 資料番号: SA1000087000
- Published
- 2008
7. Measurements of 0.2-20GeV/n cosmic-ray proton and helium spectra from 1997 through 2002 with the BESS spectrometer
- Author
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R. E. Streitmatter, Yasuhiro Makida, S. Matsuda, A. A. Moiseev, T. Yoshida, J. Suzuki, Y. Shikaze, Thomas Hams, Kazuhiro Tanaka, S. Orito, H. Fuke, K. Abe, M. Sasaki, Takamasa Yamagami, John Mitchell, Sadakazu Haino, Jonathan F. Ormes, Kohei Yoshimura, J. Nishimura, T. Sanuki, Akira Yamamoto, Mitsuaki Nozaki, K. C. Kim, and Eun-Suk Seo
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Physics ,Range (particle radiation) ,Proton ,Spectrometer ,Astrophysics (astro-ph) ,FOS: Physical sciences ,chemistry.chemical_element ,Astronomy and Astrophysics ,Cosmic ray ,Astrophysics ,Kinetic energy ,7. Clean energy ,01 natural sciences ,Spectral line ,Nuclear physics ,Atmosphere ,chemistry ,13. Climate action ,0103 physical sciences ,Nuclear Experiment ,010306 general physics ,010303 astronomy & astrophysics ,Helium - Abstract
We measured low energy cosmic-ray proton and helium spectra in the kinetic energy range 0.215 - 21.5 GeV/n at different solar activities during a period from 1997 to 2002. The observations were carried out with the BESS spectrometer launched on a balloon at Lynn Lake, Canada. A calculation for the correction of secondary particle backgrounds from the overlying atmosphere was improved by using the measured spectra at small atmospheric depths ranging from 5 through 37 g/cm^2. The uncertainties including statistical and systematic errors of the obtained spectra at the top of atmosphere are 5-7 % for protons and 6-9 % for helium nuclei in the energy range 0.5 - 5 GeV/n., Comment: 27 pages, 7 Tables, 9 figures, Submitted to Astroparticle Physics
- Published
- 2007
8. Erratum to: 'Measurements of proton, helium and muon spectra at small atmospheric depths with the BESS spectrometer' [Phys. Lett. B 564 (2003) 8]
- Author
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Yoichi Asaoka, Yasuhiro Makida, Y. Shikaze, Jun-ichi Suzuki, A. A. Moiseev, Yoshihisa Yamamoto, N. Ikeda, John Mitchell, Kazuhiro Tanaka, T. Sonoda, S. Matsuda, Mitsuaki Nozaki, T. Matsukawa, Eun-Suk Seo, Kohei Yoshimura, K. Abe, S. Orito, J. Nishimura, T. Sanuki, M. Imori, Akira Yamamoto, H. Matsumoto, K. Yamato, T. Yoshida, Keisuke Izumi, M. Sasaki, Tadashi Maeno, Nagataka Matsui, R. E. Streitmatter, Takamasa Yamagami, K. Tanizaki, Jonathan F. Ormes, Sadakazu Haino, Hideyuki Fuke, and Kazuaki Anraku
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Nuclear physics ,Physics ,Nuclear and High Energy Physics ,Muon ,Proton ,chemistry ,Spectrometer ,chemistry.chemical_element ,Atomic physics ,Helium ,Spectral line - Published
- 2007
9. The BESS Program
- Author
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Hideyuki Fuke, Thomas Hams, N. Thakur, K. Abe, Y. Shikaze, Koji Yoshimura, J. Nishimura, Reiko Orito, Sadakazu Haino, M. H. Lee, T. Sanuki, R. E. Streitmatter, T. Yoshida, S. Orito, K. Sakai, John Mitchell, K. Tanaka, Akira Yamamoto, Mitsuaki Nozaki, Y. Makida, A. A. Moiseev, S. Matsuda, J. Suzuki, M. Sasaki, Kwangmoo Kim, Takamasa Yamagami, Eun-Suk Seo, and Jonathan F. Ormes
- Subjects
Physics ,Nuclear and High Energy Physics ,Proton ,Spectrometer ,Astrophysics::High Energy Astrophysical Phenomena ,High Energy Physics::Phenomenology ,chemistry.chemical_element ,Cosmic ray ,Atomic and Molecular Physics, and Optics ,Spectral line ,Geomagnetic reversal ,Interstellar medium ,Nuclear physics ,chemistry ,Antiproton ,High Energy Physics::Experiment ,Nuclear Experiment ,Helium - Abstract
著者人数:28名, 資料番号: SA1000179000
- Published
- 2007
10. Measurement of Cosmic-Ray Proton and Antiproton Spectra at Mountain Altitude
- Author
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Kazuhiro Tanaka, Yasuhiro Makida, Hideyuki Fuke, Sadakazu Haino, Tadashi Maeno, M. Fujikawa, H. Matsumoto, Yoshihisa Yamamoto, Kazuaki Anraku, Jun-ichi Suzuki, Koji Yoshimura, Nagataka Matsui, H. Matsunaga, T. Sanuki, M. Sasaki, Tetsuya Yoshida, Keisuke Izumi, K. Yamato, M. Imori, J. Nishimura, K. Abe, S. Orito, Y. Shikaze, Mitsuaki Nozaki, and Akira Yamamoto
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Physics ,Nuclear and High Energy Physics ,Antiparticle ,Proton ,Astrophysics::High Energy Astrophysical Phenomena ,Astrophysics (astro-ph) ,Astrophysics::Instrumentation and Methods for Astrophysics ,FOS: Physical sciences ,Cosmic ray ,Astrophysics ,Baryon ,Nuclear physics ,Altitude ,Antiproton ,Antimatter ,Physics::Accelerator Physics ,High Energy Physics::Experiment ,Nuclear Experiment ,Nucleon - Abstract
著者人数: 25名, Accepted: 2003-10-08, 資料番号: SA1003537000
- Published
- 2003
11. Measurement of low-energy antiproton detection efficiency in BESS below 1
- Author
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Y. Shikaze, M. Fujikawa, Y. Makida, H. Fuke, T. Sanuki, Tetsuya Yoshida, K. Abe, Jun-ichi Suzuki, Mitsuaki Nozaki, K. Izumi, Hironori Matsumoto, Nagataka Matsui, Makoto Sasaki, T. Sonoda, Yoichi Asaoka, Koji Yoshimura, Akira Yamamoto, Kenichi Tanaka, Kazuaki Anraku, H. Matsunaga, M. Motoki, Tadashi Maeno, Y. Toki, Sadakazu Haino, and S. Orito
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Physics ,Systematic error ,Nuclear and High Energy Physics ,Physics - Instrumentation and Detectors ,Spectrometer ,High Energy Physics::Phenomenology ,Monte Carlo method ,FOS: Physical sciences ,Flux ,Instrumentation and Detectors (physics.ins-det) ,Nuclear physics ,Superconducting solenoid ,Antiproton beam ,Low energy ,Antiproton ,Physics::Accelerator Physics ,Nuclear Experiment ,Instrumentation - Abstract
著者人数: 25名, Accepted: 2002-02-14, 資料番号: SA1003532000
- Published
- 2002
12. A high-voltage power supply operating under a magnetic field
- Author
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H. Matsumoto, M. Imori, Taniguchi Tooru, H. Fuke, and Y. Shikaze
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Nuclear and High Energy Physics ,Power supply rejection ratio ,Engineering ,Switched-mode power supply ,business.industry ,Electrical engineering ,Capacitive power supply ,Voltage optimisation ,Constant power circuit ,Nuclear Energy and Engineering ,Voltage regulation ,Electrical and Electronic Engineering ,Switched-mode power supply applications ,business ,Voltage reference - Abstract
The article describes a network of high voltage power supplies where the high voltage power supply incorporates a ceramic transformer utilizing piezoelectric effect to generate high voltage. The ceramic transformer is constructed from a ceramic bar and does not include any magnetic material. So it is expected that the high voltage power supply can operate under a magnetic field. The high voltage power supply was tested under a magnetic field of 1.5 tesla. The performance of the power supply was almost intact in the magnetic field. The power supply includes feedback to stabilize the high voltage output, supplying from 1500 V to 2500 V with a load of more than 10M/spl Omega/ at a efficiency higher than 50%. From a supply voltage of 2 V, the power supply can provide about 3000 V at a load of 20 M/spl Omega/. A supply voltage of 5 V is large enough to provide 4000 V at the same load. The high voltage power supply is equipped with an interface chip with a network. Most functions of the high voltage power supply are kept under the control of the chip, and are then monitored and controlled through the network.
- Published
- 2001
13. A local network integrated into a balloon-borne apparatus
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Makoto Sasaki, Nagataka Matsui, H. Matsunaga, Takahiro Murata, Kazuaki Anraku, Takamasa Yamagami, Ikuo Ueda, Tadashi Maeno, Kotaro Shimamura, Hiroshi Matsumoto, Y. Shikaze, and M. Imori
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Interface control document ,Physics ,Nuclear and High Energy Physics ,business.industry ,Data management ,media_common.quotation_subject ,Control (management) ,Local area network ,Debugging ,Transceiver ,business ,Instrumentation ,Protocol (object-oriented programming) ,Independence (probability theory) ,Computer hardware ,media_common - Abstract
A local network is incorporated into an apparatus for a balloon-borne experiment. A balloon-borne system implemented in the apparatus is composed of subsystems interconnected through a local network, which introduces modular architecture into the system. The network decomposes the balloon-borne system into subsystems, which are similarly structured from the point of view that the systems is kept under the control of a ground station. The subsystem is functionally self-contained and electrically independent. A computer is integrated into a subsystem, keeping the subsystem under the control. An independent group of batteries, being dedicated to a subsystem, supplies the whole electricity of the subsystem. The subsystem could be turned on and off independently of the other subsystems. So communication among the subsystems needs to be based on such a protocol that could guarantee the independence of the individual subsystems. An Omninet protocol is employed to network the subsystems. A ground station sends commands to the balloon-borne system. The command is received and executed at the system, then results of the execution are returned to the ground station. Various commands are available so that the system borne on a balloon could be controlled and monitored remotely from the ground station. A subsystem responds to a specific group of commands. A command is received by a transceiver subsystem and then transferred through the network to the subsystem to which the command is addressed. Then the subsystem executes the command and returns results to the transceiver subsystem, where the results are telemetered to the ground station. The network enhances independence of the individual subsystems, which enables programs of the individual subsystems to be coded independently. Independence facilitates development and debugging of programs, improving the quality of the system borne on a balloon.
- Published
- 1998
14. Network-controlled high voltage power supply operating under magnetic field
- Author
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H. Matsumoto, M. Imori, H. Fuke, Y. Shikaze, and Taniguchi Tooru
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Engineering ,Switched-mode power supply ,business.industry ,Electrical engineering ,Hardware_PERFORMANCEANDRELIABILITY ,Power factor ,Capacitive power supply ,Voltage optimisation ,Constant power circuit ,Hardware_INTEGRATEDCIRCUITS ,Electronic engineering ,Voltage regulation ,business ,Switched-mode power supply applications ,Voltage reference - Abstract
The article describes a network of high voltage power supplies where the power supplies are controlled and managed through a network. The high voltage power supply incorporates a ceramic transformer which utilizes piezoelectric effects to generate a high voltage. The ceramic transformer is constructed from a ceramic bar and does not include any magnetic material. A high voltage power supply can work without a loss of efficiency under a magnetic field of 1.5 Tesla. The power supply includes feedback to stabilize the high voltage output, supplying from 2000V to 4000V with a load of more than 20 megohm at efficiency higher than 50 percent. The high voltage power supply includes a Neuron chip, a programming device processing a variety of input and output capabilities. The chip can also communicate with other Neuron chips over a twisted-pair cable, which allows establishing a high voltage control network consisting of a number of power supplies that incorporate the chip individually. The functions of the power supply under the control of the chip are managed through the network. The chip turns on and off the high voltage power supply and sets the output high voltage. The chip detects the short circuit of the output high voltage and controls its recovery. The chip also monitors the output current. Thus the high voltage power supplies are monitored and controlled through the network.
- Published
- 2005
15. A high voltage power supply operating under a magnetic field
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Y. Shikaze, M. Imori, H. Fuke, H. Matsumoto, and T. Taniguchi
- Published
- 2002
16. Measurements of atmospheric muon spectra at mountain altitude
- Author
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Hideyuki Fuke, Kenichi Tanaka, K. Abe, Y. Makida, Kazuaki Anraku, Hironori Matsumoto, M. Motoki, K. Izumi, T. Sanuki, Y. Yamamoto, Sadakazu Haino, T. Sonoda, Tadashi Maeno, Akira Yamamoto, Masatoshi Imori, H. Matsunaga, Koji Yoshimura, Mitsuaki Nozaki, J. Nishimura, Yoichi Asaoka, S. Orito, Nagataka Matsui, Y. Shikaze, Y. Toki, K. Yamato, Jun-ichi Suzuki, M. Fujikawa, Takashi Yoshida, and Makoto Sasaki
- Subjects
Physics ,Nuclear and High Energy Physics ,Muon ,Physics::Instrumentation and Detectors ,Detector ,Astrophysics (astro-ph) ,FOS: Physical sciences ,Astrophysics ,Atmospheric sciences ,Spectral line ,Altitude ,High Energy Physics::Experiment ,Astrophysics::Earth and Planetary Astrophysics ,Atmospheric neutrino ,Sea level ,Physics::Atmospheric and Oceanic Physics - Abstract
We report new measurements of the atmospheric muons at mountain altitude. The measurement was carried out with the BESS detector at the top of Mt. Norikura, Japan. The altitude is 2,770 m above sea level. Comparing our results and predictions given by some interaction models, a further appropriate model has been investigated. These studies would improve accuracy of atmospheric neutrino calculations., Comment: Mean momentum in Table 1 was corrected
- Published
- 2002
- Full Text
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17. Large-Area Scintillator Hodoscope with 50 ps Timing Resolution Onboard BESS
- Author
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Hiroshi Matsumoto, Koji Yoshimura, T. Mitsui, H. Matsunaga, Y. Shikaze, S. Orito, Mitsuaki Nozaki, T. Sonoda, Tetsuya Yoshida, and Ikuo Ueda
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Physics ,Nuclear and High Energy Physics ,Photomultiplier ,Particle physics ,Muon ,Spectrometer ,business.industry ,Physics::Instrumentation and Detectors ,Gaussian ,FOS: Physical sciences ,Scintillator ,Photoelectric effect ,High Energy Physics - Experiment ,Magnetic field ,symbols.namesake ,High Energy Physics - Experiment (hep-ex) ,Optics ,Hodoscope ,symbols ,business ,Instrumentation - Abstract
We describe the design and performance of a large-area scintillator hodoscope onboard the BESS rigidity spectrometer; an instrument with an acceptance of 0.3 m^{2}sr. The hodoscope is configured such that 10 and 12 counters are respectively situated in upper and lower layers. Each counter is viewed from its ends by 2.5 inch fine-mesh photomultiplier tubes placed in a stray magnetic field of 0.2 Tesla. Various beam-test data are presented. Use of cosmic-ray muons at ground-level confirmed 50 ps timing resolution for each layer, giving an overall time-of-flight resolution of 70 ps rms using a pure Gaussian resolution function. Comparison with previous measurements on a similar scintillator hodoscope indicates good agreement with the scaling law that timing resolution is proportional to 1/$\sqrt{N_{\rm pe}}$, where $N_{\rm pe}$ is the effective number of photoelectrons., Comment: 16 pages, 14 figures
- Published
- 2000
- Full Text
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18. Erratum to: 'Measurements of atmospheric muon spectra at mountain altitude'
- Author
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Yoshihisa Yamamoto, Hideyuki Fuke, Akira Yamamoto, Yasuhiro Makida, K. Yamato, Y. Shikaze, Kazuaki Anraku, T. Sonoda, Kohei Yoshimura, H. Matsunaga, Nagataka Matsui, Keisuke Izumi, H. Matsumoto, M. Imori, Jun-ichi Suzuki, J. Nishimura, T. Sanuki, Mitsuaki Nozaki, K. Abe, T. Yoshida, Yoichi Asaoka, M. Sasaki, Kazuhiro Tanaka, Y. Toki, S. Orito, Sadakazu Haino, M. Motoki, Tadashi Maeno, and M. Fujikawa
- Subjects
Physics ,Nuclear and High Energy Physics ,Altitude ,Muon ,Atmospheric sciences ,Spectral line - Published
- 2004
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19. Measurements of cosmic-ray proton and helium spectra from the BESS-Polar long-duration balloon flights over Antarctica.
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Abe K, Fuke H, Haino S, Hams T, Hasegawa M, Horikoshi A, Itazaki A, Kim KC, Kumazawa T, Kusumoto A, Lee MH, Makida Y, Matsuda S, Matsukawa Y, Matsumoto K, Mitchell JW, Myers Z, Nishimura J, Nozaki M, Orito R, Ormes JF, Picot-Clemente N, Sakai K, Sasaki M, Seo ES, Shikaze Y, Shinoda R, Streitmatter RE, Suzuki J, Takasugi Y, Takeuchi K, Tanaka K, Thakur N, Yamagami T, Yamamoto A, Yoshida T, and Yoshimura K
- Abstract
The BESS-Polar Collaboration measured the energy spectra of cosmic-ray protons and helium during two long-duration balloon flights over Antarctica in December 2004 and December 2007, at substantially different levels of solar modulation. Proton and helium spectra probe the origin and propagation history of cosmic rays in the galaxy, and are essential to calculations of the expected spectra of cosmic-ray antiprotons, positrons, and electrons from interactions of primary cosmic-ray nuclei with the interstellar gas, and to calculations of atmospheric muons and neutrinos. We report absolute spectra at the top of the atmosphere for cosmic-ray protons in the kinetic energy range 0.2-160 GeV and helium nuclei 0.15-80 GeV/nucleon. The corresponding magnetic rigidity ranges are 0.6-160 GV for protons and 1.1-160 GV for helium. These spectra are compared to measurements from previous BESS flights and from ATIC-2, PAMELA, and AMS-02. We also report the ratio of the proton and helium fluxes from 1.1 GV to 160 GV and compare to ratios from PAMELA and AMS-02.
- Published
- 2016
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20. Search for antihelium with the BESS-Polar spectrometer.
- Author
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Abe K, Fuke H, Haino S, Hams T, Hasegawa M, Horikoshi A, Itazaki A, Kim KC, Kumazawa T, Kusumoto A, Lee MH, Makida Y, Matsuda S, Matsukawa Y, Matsumoto K, Mitchell JW, Myers Z, Nishimura J, Nozaki M, Orito R, Ormes JF, Sakai K, Sasaki M, Seo ES, Shikaze Y, Shinoda R, Streitmatter RE, Suzuki J, Takasugi Y, Takeuchi K, Tanaka K, Thakur N, Yamagami T, Yamamoto A, Yoshida T, and Yoshimura K
- Abstract
In two long-duration balloon flights over Antarctica, the Balloon-borne Experiment with a Superconducting Spectrometer (BESS) collaboration has searched for antihelium in the cosmic radiation with the highest sensitivity reported. BESS-Polar I flew in 2004, observing for 8.5 days. BESS-Polar II flew in 2007-2008, observing for 24.5 days. No antihelium candidate was found in BESS-Polar I data among 8.4×10(6) |Z|=2 nuclei from 1.0 to 20 GV or in BESS-Polar II data among 4.0×10(7) |Z|=2 nuclei from 1.0 to 14 GV. Assuming antihelium to have the same spectral shape as helium, a 95% confidence upper limit to the possible abundance of antihelium relative to helium of 6.9×10(-8)} was determined combining all BESS data, including the two BESS-Polar flights. With no assumed antihelium spectrum and a weighted average of the lowest antihelium efficiencies for each flight, an upper limit of 1.0×10(-7) from 1.6 to 14 GV was determined for the combined BESS-Polar data. Under both antihelium spectral assumptions, these are the lowest limits obtained to date.
- Published
- 2012
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21. Construction of monoenergetic neutron calibration fields using 45Sc(p, n)45Ti reaction at JAEA.
- Author
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Tanimura Y, Saegusa J, Shikaze Y, Tsutsumi M, Shimizu S, and Yoshizawa M
- Subjects
- Calibration, Equipment Design, Equipment Failure Analysis, Japan, Radioisotopes standards, Reference Standards, Scandium standards, Titanium standards, Neutrons, Radioisotopes analysis, Radiometry instrumentation, Radiometry standards, Scandium analysis, Titanium analysis
- Abstract
The 8 and 27 keV monoenergetic neutron calibration fields have been developed by using (45)Sc(p, n)(45)Ti reaction. Protons from a 4-MV Pelletron accelerator are used to bombard a thin scandium target evaporated onto a platinum disc. The proton energies are finely adjusted to the resonance to generate the 8 and 27 keV neutrons by applying a high voltage to the target assemblies. The neutron energies were measured using the time-of-flight method with a lithium glass scintillation detector. The neutron fluences at a calibration point located at 50 cm from the target were evaluated using Bonner spheres. A long counter was placed at 2.2 m from the target and at 60 degrees to the direction of the proton beam in order to monitor the fluence at the calibration point. Fluence and dose equivalent rates at the calibration point are sufficient to calibrate many types of the neutron survey metres.
- Published
- 2007
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22. Investigation of properties of the TIARA neutron beam facility of importance for calibration applications.
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Shikaze Y, Tanimura Y, Saegusa J, Tsutsumi M, Yamaguchi Y, and Uchita Y
- Subjects
- Calibration, Equipment Design, Equipment Failure Analysis, Japan, Radiation Dosage, Neutrons, Particle Accelerators instrumentation, Particle Accelerators standards, Radiometry instrumentation, Radiometry standards
- Abstract
Evaluation of the properties for quasi-monoenergetic neutron calibration fields of high energies more than 20 MeV at TIARA is proceeding for development of the field. Among the properties needed for the development as the standard calibration field, we report on measurement of the neutron beam profile using an imaging plate with a polyethylene converter and on estimation of the contribution of scattered neutrons into the irradiation field based on pulse height distribution at various off-beam positions measured using an organic liquid scintillation detector.
- Published
- 2007
- Full Text
- View/download PDF
23. Search for cosmic-ray antideuterons.
- Author
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Fuke H, Maeno T, Abe K, Haino S, Makida Y, Matsuda S, Matsumoto H, Mitchell JW, Moiseev AA, Nishimura J, Nozaki M, Orito S, Ormes JF, Sasaki M, Seo ES, Shikaze Y, Streitmatter RE, Suzuki J, Tanaka K, Tanizaki K, Yamagami T, Yamamoto A, Yamamoto Y, Yamato K, Yoshida T, and Yoshimura K
- Abstract
We performed a search for cosmic-ray antideuterons using data collected during four BESS balloon flights from 1997 to 2000. No candidate was found. We derived, for the first time, an upper limit of 1.9 x 10(-4) (m2s sr GeV/nucleon)(-1) for the differential flux of cosmic-ray antideuterons, at the 95% confidence level, between 0.17 and 1.15 GeV/nucleon at the top of the atmosphere.
- Published
- 2005
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24. Measurements of cosmic-ray low-energy antiproton and proton spectra in a transient period of solar field reversal.
- Author
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Asaoka Y, Shikaze Y, Abe K, Anraku K, Fujikawa M, Fuke H, Haino S, Imori M, Izumi K, Maeno T, Makida Y, Matsuda S, Matsui N, Matsukawa T, Matsumoto H, Matsunaga H, Mitchell J, Mitsui T, Moiseev A, Motoki M, Nishimura J, Nozaki M, Orito S, Ormes JF, Saeki T, Sanuki T, Sasaki M, Seo ES, Sonoda T, Streitmatter R, Suzuki J, Tanaka K, Tanizaki K, Ueda I, Wang JZ, Yajima Y, Yamagami Y, Yamamoto A, Yamamoto Y, Yamato K, Yoshida T, and Yoshimura K
- Abstract
The energy spectra of cosmic-ray low-energy antiprotons ( *p's) and protons ( p's) have been measured by BESS in 1999 and 2000, during a period covering reversal at the solar magnetic field. Based on these measurements, a sudden increase of the *p/p flux ratio following the solar magnetic field reversal was observed, and it generally agrees with a drift model of the solar modulation.
- Published
- 2002
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25. Precision measurement of cosmic-Ray antiproton spectrum
- Author
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Orito S, Maeno T, Matsunaga H, Abe K, Anraku K, Asaoka Y, Fujikawa M, Imori M, Ishino M, Makida Y, Matsui N, Matsumoto H, Mitchell J, Mitsui T, Moiseev A, Motoki M, Nishimura J, Nozaki M, Ormes J, Saeki T, Sanuki T, Sasaki M, Seo ES, Shikaze Y, Sonoda T, and Streitmatter R
- Abstract
The energy spectrum of cosmic-ray antiprotons ( &pmacr;'s) has been measured in the range 0.18-3.56 GeV, based on 458 &pmacr;'s collected by BESS in a recent solar-minimum period. We have detected for the first time a characteristic peak at 2 GeV of &pmacr;'s originating from cosmic-ray interactions with the interstellar gas. The peak spectrum is reproduced by theoretical calculations, implying that the propagation models are basically correct and that different cosmic-ray species undergo a universal propagation. Future BESS data with still higher statistics will allow us to study the solar modulation and the propagation in detail and to search for primary &pmacr; components.
- Published
- 2000
- Full Text
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