Measurement of the cosmic-ray antiproton spectrum in the range 0.12 to 0.4 GeV with BESS-Polar II

The energy spectra of cosmic-ray antiprotons and protons near solar minimum were precisely measured with BESS-Polar II (Balloon-borne Experiment with a Superconducting Spectrometer) during a long-duration flight over Antarctica in December 2007 and January 2008. The upper-TOF (UTOF) and lower-TOF (L...

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Bibliographic Details
Main Authors: Sakai, K, Abe, JK, Fuke, H, Haino, S, Hams, T, Hasegawa, M, Kim, KC, Lee, MH, Makida, Y, Mitchell, JW, Nishimura, J, Nozaki, M, Orito, R, Ormes, JF, Picot-Clemente, N, Sasaki, M, Seo, ES, Streitmatter, RE, Suzuki, J, Tanaka, K, Thakur, N, Yamamoto, A, Yoshida, T, Yoshimura, K
Format: Report
Language:English
Published: Proceedings of Science 2017
Subjects:
Antarc*
Antarctica
Online Access:https://discovery.ucl.ac.uk/id/eprint/10048832/1/ICRC2017_174.pdf
https://discovery.ucl.ac.uk/id/eprint/10048832/
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Summary:The energy spectra of cosmic-ray antiprotons and protons near solar minimum were precisely measured with BESS-Polar II (Balloon-borne Experiment with a Superconducting Spectrometer) during a long-duration flight over Antarctica in December 2007 and January 2008. The upper-TOF (UTOF) and lower-TOF (LTOF) scintillator hodoscopes measure the charge and velocity of incident particles. A thin plastic scintillator middle-TOF (MTOF) hodoscope is installed on the lower surface of the magnet bore to measure low-energy particles that cannot reach the LTOF. The MTOF further lowers the threshold energy to about 120 MeV for antiproton or proton measurements. We report absolute spectra of the cosmic-ray antiproton in the range 0.12 to 0.4 GeV and the antiproton/proton ratio calculated with UTOF-MTOF trigger events. These new results are independent of the UTOF-LTOF triggered antiproton spectrum published in 2012 and proton spectrum published in 2016.

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