AbstractThe Balloon Borne Experiment with a Superconducting Spectrometer (BESS) has measured the energy spectrum of cosmic-ray antiprotons between 0.18 and 4.20 GeV in eight flights between 1993 and 2002. Above about 1 GeV, models in which antiprotons are secondary products of the interactions of primary cosmic rays with the interstellar gas agree with the BESS antiproton spectrum. Below 1 GeV, the data show a possible excess antiproton flux compared to secondary model predictions, suggesting the presence of an additional source of antiprotons. The antiproton/proton ratios measured between 1993 and 1999, during the Sun’s positive-polarity phase, are consistent with simple models of solar modulation. However, results from the 2000 flight, following the solar magnetic field reversal, show a sudden increase in the antiproton/proton ratio and tend to favor a charge-sign-dependent drift model. To extend BESS measurements to lower energies, an evolutionary instrument, BESS-Polar, is under construction for polar flight in 2004.


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    Title :

    Precise measurements of the cosmic ray antiproton spectrum with BESS including the effects of solar modulation


    Contributors:
    Mitchell, J.W. (author) / Abe, K. (author) / Anraku, K. (author) / Asaoka, Y. (author) / Fujikawa, M. (author) / Fuke, H. (author) / Haino, S. (author) / Hams, T. (author) / Ikeda, N. (author) / Imori, M. (author)

    Published in:

    Advances in Space Research ; 35 , 1 ; 135-141


    Publication date :

    2003-08-14


    Size :

    7 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English




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