activity
20122026
most citedThe cosmic-ray positron energy spectrum measured by PAMELA

308 citations · 1k across the 42 of their papers we have counts for

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Showing 2015Show all

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astro-ph.HE2015★ 74 cited

Measurements of Cosmic-Ray Hydrogen and Helium Isotopes with the PAMELA experiment

O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +56

The cosmic-ray hydrogen and helium (H, H, He, He) isotopic composition has been measured with the satellite-borne experiment PAMELA, which was launched into low-Ear…

astro-ph.EP2015★ 6 cited

PAMELA's measurements of geomagnetically trapped and albedo protons

A. Bruno, O. Adriani, G. C. Barbarino +64

Data from the PAMELA satellite experiment were used to perform a detailed measurement of under-cutoff protons at low Earth orbits. On the basis of a trajectory tracing approach usi…

astro-ph.EP2015★ 3 cited

PAMELA's measurements of geomagnetic cutoff variations during solar energetic particle events

A. Bruno, O. Adriani, G. C. Barbarino +64

Data from the PAMELA satellite experiment were used to measure the geomagnetic cutoff for high-energy ( 80 MeV) protons during the solar particle events on 2006 December 1…

astro-ph.HE2015★ 16 cited

Search for anisotropies in cosmic-ray positrons detected by the PAMELA experiment

O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +57

The PAMELA detector was launched on board of the Russian Resurs-DK1 satellite on June 15, 2006. Data collected during the first four years have been used to search for large-scale…

astro-ph.HE2015

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…

astro-ph.SR2015★ 44 cited

PAMELA's Measurements of Magnetospheric Effects on High Energy Solar Particles

O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +64

The nature of particle acceleration at the Sun, whether through flare reconnection processes or through shocks driven by coronal mass ejections (CMEs), is still under scrutiny desp…