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Observation of an anomalous positron abundance in the cosmic radiation, , , , , , , , , and 41 other author(s). (2008)cite arxiv:0810.4995 Comment: Submitted to Nature, 20 pages, 5 figures, 1 table.Supporting interactive workflow systems through graphical web interfaces and interactive simulators., , and . TAMODIA, page 63-70. ACM, (2005)Measurement of the flux of primary cosmic ray antiprotons with energies of 60 MeV to 350 GeV in the PAMELA experiment, , , , , , , , , and 58 other author(s). JETP Letters, 96 (10): 621--627 (Jan 1, 2013)Measurements of cosmic-ray proton and helium spectra with the PAMELA calorimeter, , , , , , , , , and 49 other author(s). Advances in Space Research, 51 (2): 219--226 (January 2013)New Measurement of the Antiproton-to-Proton Flux Ratio up to 100 GeV in the Cosmic Radiation, , , , , , , , , and 43 other author(s). Phys. Rev. Lett., 102 (5): 051101 (February 2009)PAMELA and electrons, , , , , , , , , and 50 other author(s). Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 630 (1): 28 - 35 (2011)Proceedings of the 2nd Roma International Conference on Astroparticle Physics (RICAP 2009).PAMELA'S MEASUREMENTS OF MAGNETOSPHERIC EFFECTS ON HIGH-ENERGY SOLAR PARTICLES, , , , , , , , , and 57 other author(s). The Astrophysical Journal, 801 (1): L3 (February 2015)TIME DEPENDENCE OF THE PROTON FLUX MEASURED BY PAMELA DURING THE 2006 JULY-2009 DECEMBER SOLAR MINIMUM, , , , , , , , , and 54 other author(s). The Astrophysical Journal, 765 (2): 91 (February 2013)Analysis on H spectral shape during the early 2012 SEPs with the PAMELA experiment, , , , , , , , , and 59 other author(s). Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, (2014)4th Roma International Conference on Astroparticle Physics.PAMELA Results on the Cosmic-Ray Antiproton Flux from 60 MeV to 180 GeV in Kinetic Energy, , , , , , , , , and 53 other author(s). Phys. Rev. Lett., 105 (12): 121101 (September 2010)