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The CAESAR Project for the ASI Space Weather Infrastructure., , , , , , , , , and 85 other author(s). Remote. Sens., 15 (2): 346 (January 2023)THE DISCOVERY OF GEOMAGNETICALLY TRAPPED COSMIC-RAY ANTIPROTONS, , , , , , , , , and 54 other author(s). The Astrophysical Journal, 737 (2): L29 (July 2011)Results from PAMELA, , , , , , , , , and 57 other author(s). Nuclear Physics B - Proceedings Supplements, 217 (1): 243 - 248 (2011)Proceedings of the Neutrino Oscillation Workshop (NOW 2010).Anisotropy studies in the cosmic ray proton flux with the PAMELA experiment, , , , , , , , , and 59 other author(s). Nuclear Physics B - Proceedings Supplements, (June 2013)OBSERVATIONS OF THE 2006 DECEMBER 13 AND 14 SOLAR PARTICLE EVENTS IN THE 80 MeV n–1-3 GeV n–1RANGE FROM SPACE WITH THE PAMELA DETECTOR, , , , , , , , , and 55 other author(s). The Astrophysical Journal, 742 (2): 102 (November 2011)Measurements of quasi-trapped electron and positron fluxes with PAMELA, , , , , , , , , and 56 other author(s). Journal of Geophysical Research: Space Physics, (2009)PAMELA Measurements of Cosmic-Ray Proton and Helium Spectra, , , , , , , , , and 55 other author(s). Science, 332 (6025): 69--72 (2011)Cosmic-Ray Electron Flux Measured by the PAMELA Experiment between 1 and 625 GeV, , , , , , , , , and 56 other author(s). Phys. Rev. Lett., 106 (20): 201101 (May 2011)Deep Learning LSTM-based approaches for 10.7 cm solar radio flux forecasting up to 45-days., and . Astron. Comput., (January 2024)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)