activity
19952023
most citedMeasurements of 0.2 to 20 GeV/n cosmic-ray proton and helium spectra from 1997 through 2002 with the BESS spectrometer

203 citations · 1k across the 30 of their papers we have counts for

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astro-ph2008★ 106 cited

Measurement of cosmic-ray low-energy antiproton spectrum with the first BESS-Polar Antarctic flight

K. Abe, H. Fuke, S. Haino +27

The BESS-Polar spectrometer had its first successful balloon flight over Antarctica in December 2004. During the 8.5-day long-duration flight, almost 0.9 billion events were record…

astro-ph2006★ 203 cited

Measurements of 0.2 to 20 GeV/n cosmic-ray proton and helium spectra from 1997 through 2002 with the BESS spectrometer

Y. Shikaze, S. Haino, K. Abe +21

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 obse…

astro-ph2005★ 10 cited

Measurements of Atmospheric Antiprotons

K. Yamato, K. Abe, H. Fuke +21

We measured atmospheric antiproton spectra in the energy range 0.2 to 3.4 GeV, at sea level and at balloon altitude in the atmospheric depth range 4.5 to 26 g/cm^2. The observed en…

astro-ph2005★ 113 cited

Search for Cosmic-Ray Antideuterons

H. Fuke, T. Maeno, K. Abe +23

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,…

astro-ph2003

Measurement of Cosmic-Ray Proton, Antiproton and Muon Spectra at Mountain Altitude

T. Sanuki, M. Fujikawa, K. Abe +22

Measurement of cosmic-ray proton, antiproton and muon spectra was carried out at mountain altitude. We observed 2 x 10^5 protons and 10^2 antiprotons in a kinetic energy region of…

astro-ph2002★ 63 cited

Precise Measurements of Atmospheric Muon Fluxes with the BESS Spectrometer

M. Motoki, T. Sanuki, S. Orito +36

The vertical absolute fluxes of atmospheric muons and muon charge ratio have been measured precisely at different geomagnetic locations by using the BESS spectrometer. The observat…