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The PAMELA satellite has observed an excess in the positron to electron ratio above theoretical predictions in the range 10 - 100 GeV that increases with energy.
Dynamics of the interplanetary gas and magnetic fields
E. N Parker · 1958
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The passage of energetic charged particles through interplanetary space
E. N Parker · 1965
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Origin of the twenty year wave in the diurnal variation
E Levy · 1975
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The calculation of neutral sheet drift in two-dimensional cosmic-ray modulation models
R. A Burger and M. S Potgieter · 1989
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The large-scale structure of the heliospheric current sheet during the ulysses epoch
J. Todd Hoeksema · 1995
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Motion of the footpoints of heliospheric magnetic field lines at the sun: Implications for recurrent energetic particle events at high heliographic latitudes
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Andrew W Strong and Igor V Moskalenko · 1998
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An anomalous positron abundance in cosmic rays with energies 1.5–100 gev
O Adriani, G Barbarino, and G Bazilevskaya · 2009
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Solar cycle variations of heliospheric magnetic flux
Xiaoyan Zhou and Edward J Smith · 2009
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Mixdm: Cosmic ray signals from multiple states of dark matter
Ilias Cholis and Neal Weiner · 2009
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Theory of the solar magnetic cycle wave in the diurnal variation of energetic cosmic rays - physical basis of the anisotropy
E Levy · 2088
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http://wso.stanford.edu/tilts.html
Wilcox Solar Observatory
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