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Adriani, O. et al. (2011). PAMELA Measurements of Cosmic- Ray Proton and Helium Spectra. Science, 332, 69–71 Adriani, O. et al. (2011). Observations of the December 13 and 14, 2006, Solar Particle Events in the 80 MeV/n – 3 GeV/n range from space with PAMELA detector. ApJ 742, 102. PAMELA Collaboration (2010). PAMELA results on the cosmic- ray antiproton flux from 60 MeV to 180 GeV in kinetic energy. PRL, 105, 121101. Adriani, O. et al. (2011). The Discovery of Geomagnetically Trapped Cosmic-ray Antiprotons. ApJ, 737, L29+. Adriani, O. et al. (2011). Cosmic-Ray Electron Flux Measured by the PAMELA Experiment between 1 and 625 GeV. PRL, 106(20), 201101 Adriani, O. et al. (2009). An anomalous positron abundance

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Adriani, O. et al. (2011). PAMELA Measurements of Cosmic-Ray Proton and Helium Spectra. Science , 332, 69–71 Adriani, O. et al. (2011). Observations of the December 13 and 14, 2006, Solar Particle Events in the 80 MeV/n – 3 GeV/n range from space with PAMELA detector. ApJ 742, 102. - PowerPoint PPT Presentation

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Page 1: AMS-02

Adriani, O. et al. (2011). PAMELA Measurements of Cosmic-Ray Proton and Helium Spectra. Science, 332, 69–71Adriani, O. et al. (2011). Observations of the December 13 and 14, 2006, Solar Particle Events in the 80 MeV/n – 3 GeV/n range from space with PAMELA detector. ApJ 742, 102.PAMELA Collaboration (2010). PAMELA results on the cosmic-ray antiproton flux from 60 MeV to 180 GeV in kinetic energy. PRL, 105, 121101.Adriani, O. et al. (2011). The Discovery of Geomagnetically Trapped Cosmic-ray Antiprotons. ApJ, 737, L29+.Adriani, O. et al. (2011). Cosmic-Ray Electron Flux Measured by the PAMELA Experiment between 1 and 625 GeV. PRL, 106(20), 201101Adriani, O. et al. (2009). An anomalous positron abundance in cosmic rays with energies 1.5-100 GeV. Nature, 458(7238), 607–609

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Athay, R. G. and Moreton, G. E.: 1961, ApJ 133, 935.

Moreton Wave, Dec 6th 2006 (from Ed Cliver)