15 research outputs found
Measurement of low-energy antiproton detection efficiency in BESS below 1 GeV
An accelerator experiment was performed using a low-energy antiproton beam to
measure antiproton detection efficiency of BESS, a balloon-borne spectrometer
with a superconducting solenoid. Measured efficiencies showed good agreement
with calculated ones derived from the BESS Monte Carlo simulation based on
GEANT/GHEISHA. With detailed verification of the BESS simulation, the relative
systematic error of detection efficiency derived from the BESS simulation has
been determined to be 5%, compared with the previous estimation of
15% which was the dominant uncertainty for measurements of cosmic-ray
antiproton flux.Comment: 13 pages, 7 figure
Precise Measurement of Cosmic-Ray Proton and Helium Spectra with the BESS Spectrometer
We report cosmic-ray proton and helium spectra in energy ranges of 1 to 120
GeV and 1 to 54 GeV/nucleon, respectively, measured by a balloon flight of the
BESS spectrometer in 1998. The magnetic-rigidity of the cosmic-rays was
reliably determined by highly precise measurement of the circular track in a
uniform solenoidal magnetic field of 1 Tesla. Those spectra were determined
within overall uncertainties of +-5 % for protons and +- 10 % for helium nuclei
including statistical and systematic errors.Comment: 12 pages, 4 figure
Measurements of atmospheric muon spectra at mountain altitude
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 correcte
Measurements of Cosmic-ray Low-energy Antiproton and Proton Spectra in a Transient Period of the Solar Field Reversal
The energy spectra of cosmic-ray low-energy antiprotons and protons have been
measured by BESS in 1999 and 2000, during a period covering the solar magnetic
field reversal. Based on these measurements, a sudden increase of the
antiproton to proton flux ratio following the solar magnetic field reversal was
observed, and it generally agrees with a drift model of the solar modulation.Comment: 4 pages, 4 figures, revised version accepted for publication in Phys.
Rev. Let