首页 | 本学科首页   官方微博 | 高级检索  
     检索      


Time variations of cosmic-ray helium isotopes with BESS-Polar I
Authors:K Abe  H Fuke  S Haino  T Hams  M Hasegawa  A Horikoshi  A Itazaki  KC Kim  T Kumazawa  A Kusumoto  MH Lee  Y Makida  S Matsuda  Y Matsukawa  K Matsumoto  JW Mitchell  AA Moiseev  J Nishimura  M Nozaki  R Orito  JF Ormes  N Picot-Clémente  K Sakai  M Sasaki  ES Seo  Y Shikaze  R Shinoda  RE Streitmatter  J Suzuki  Y Takasugi  K Takeuchi  K Tanaka  N Thakur  T Yamagami  A Yamamoto  T Yoshida  K Yoshimura
Institution:1. Kobe University, Kobe, Hyogo 657-8501, Japan;2. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA), Sagamihara, Kanagawa 252-5210, Japan;3. High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan;4. National Aeronautics and Space Administration, Goddard Space Flight Center (NASA/GFSC), Greenbelt, MD 20771, USA;5. Institute for Physical Science and Technology (IPST), University of Maryland, College Park, MD 20742, USA;6. University of Denver, Denver, CO 80208, USA;g The University of Tokyo, Bunkyo, Tokyo 113-0033, Japan
Abstract:The Balloon-borne Experiment with a Superconducting Spectrometer (BESS) is configured with a solenoidal superconducting magnet and a suite of precision particle detectors, including time-of-flight hodoscopes based on plastic scintillators, a silica-aerogel Cherenkov detector, and a high resolution tracking system with a central jet-type drift chamber. The charges of incident particles are determined from energy losses in the scintillators. Their magnetic rigidities (momentum/charge) are measured by reconstructing each particle trajectory in the magnetic field, and their velocities are obtained by using the time-of-flight system. Together, these measurements can accurately identify helium isotopes among the incoming cosmic-ray helium nuclei up to energies in the GeV per nucleon region. The BESS-Polar I instrument flew for 8.5 days over Antarctica from December 13th to December 21st, 2004. Its long-duration flight and large geometric acceptance allow the time variations of isotopic fluxes to be studied for the first time. The time variations of helium isotope fluxes are presented here for rigidities from 1.2 to 2.5 GV and results are compared to previously reported proton data and neutron monitor data.
Keywords:Cosmic-ray isotopes  Cosmic-ray flux time variations  Solar modulation  Solar activity
本文献已被 ScienceDirect 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号