440 citations · 1k across the 8 of their papers we have counts for
8 papers
PAMELA's measurements of geomagnetic cutoff variations during the 14 December 2006 storm
O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +55
Data from the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA) satellite experiment were used to measure the geomagnetic cutoff for high-energy (>80…
Solar energetic particle events: trajectory analysis and flux reconstruction with PAMELA
A. Bruno, O. Adriani, G. C. Barbarino +64
The PAMELA satellite experiment is providing first direct measurements of Solar Energetic Particles (SEPs) with energies from about 80 MeV to several GeV in near-Earth space, bridg…
Re-Entrant Albedo Proton Fluxes Measured by the PAMELA Experiment
O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +56
We present a precise measurement of downward-going albedo proton fluxes for kinetic energy above 70 MeV performed by the PAMELA experiment at an altitude between 350 and 610…
Measurement of the isotopic composition of hydrogen and helium nuclei in cosmic rays with the PAMELA experiment
O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +59
The satellite-borne experiment PAMELA has been used to make new measurements of cosmic ray H and He isotopes. The isotopic composition was measured between 100 and 600 MeV/n for hy…
Time dependence of the proton flux measured by PAMELA during the July 2006 - December 2009 solar minimum
O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +61
The energy spectra of galactic cosmic rays carry fundamental information regarding their origin and propagation. These spectra, when measured near Earth, are significantly affected…
A statistical procedure for the identification of positrons in the PAMELA experiment
O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +58
The PAMELA satellite experiment has measured the cosmic-ray positron fraction between 1.5 GeV and 100 GeV. The need to reliably discriminate between the positron signal and proton…