Measurements of Cosmic-ray Low-energy Antiproton and Proton Spectra in a Transient Period of the Solar Field Reversal

Details Measurements of Cosmic-ray Low-energy Antiproton and Proton Spectra in a Transient Period of the Solar Field Reversal Measurements of Cosmic-ray Low-energy Antiproton and Proton Spectra in a Transient Period of the Solar Field Reversal

2001-09-02

arxiv.org/abs/astro-ph/0109007v2

Phys.Rev.Lett.88:051101,2002

Astronomy and Astrophysics

Astrophysics

4 pages, 4 figures, revised version accepted for publication in Phys. Rev. Lett

Scientific paper

10.1103/PhysRevLett.88.051101

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.

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