activity
20132025
most citedThe cosmic-ray positron energy spectrum measured by PAMELA

308 citations · 834 across the 20 of their papers we have counts for

collaborators

20 papers

physics.ins-det2025

Control and read-out of the HEPD-02 tracking system onboard CSES-02 satellite

S. Bartocci, R. Battiston, S. Beolè +42

The High Energy Particle Detector (HEPD-02) is a payload of the second China Seismo-Electromagnetic Satellite (CSES-02), designed and built by the Italian Limadou collaboration. It…

astro-ph.HE2023

Gamma-Ray Burst observations by the high-energy charged particle detector on board the CSES-01 satellite between 2019 and 2021

Francesco Palma, Matteo Martucci, Coralie Neubüser +68

In this paper we report the detection of five strong Gamma-Ray Bursts (GRBs) by the High-Energy Particle Detector (HEPD-01) mounted on board the China Seismo-Electromagnetic Satell…

astro-ph.HE2022★ 23 cited

Helium fluxes measured by the PAMELA experiment from the minimum to the maximum solar activity for solar cycle 24

N. Marcelli, M. Boezio, A. Lenni +53

Time-dependent energy spectra of galactic cosmic rays (GCRs) carry fundamental information regarding their origin and propagation. When observed at the Earth, these spectra are sig…

astro-ph.SR2021★ 17 cited

Solar-Cycle Variations of South-Atlantic Anomaly Proton Intensities Measured With The PAMELA Mission

A. Bruno, M. Martucci, F. S. Cafagna +50

We present a study of the solar-cycle variations of >80 MeV proton flux intensities in the lower edge of the inner radiation belt, based on the measurements of the Payload for Anti…

astro-ph.HE2020★ 33 cited

Time dependence of the flux of helium nuclei in cosmic rays measured by the PAMELA experiment between July 2006 and December 2009

N. Marcelli, M. Boezio, A. Lenni +53

Precise time-dependent measurements of the Z = 2 component in the cosmic radiation provide crucial information about the propagation of charged particles through the heliosphere. T…

astro-ph.SR2018★ 90 cited

Solar energetic particle events observed by the PAMELA mission

A. Bruno, G. A. Bazilevskaya, M. Boezio +55

Despite the significant progress achieved in recent years, the physical mechanisms underlying the origin of solar energetic particles (SEPs) are still a matter of debate. The compl…

astro-ph.HE2018★ 24 cited

Lithium and Beryllium isotopes with the PAMELA experiment

W. Menn, E. A. Bogomolov, M. Simon +56

The cosmic-ray lithium and beryllium (Li, Li, Be, Be, Be) isotopic composition has been measured with the satellite-borne experiment PAMELA, which wa…

astro-ph.HE2018★ 34 cited

Evidence of energy and charge sign dependence of the recovery time for the December 2006 Forbush event measured by the PAMELA experiment

R. Munini, M. Boezio, A. Bruno +55

New results on the short-term galactic cosmic ray (GCR) intensity variation (Forbush decrease) in December 2006 measured by the PAMELA instrument are presented. Forbush decreases a…

astro-ph.HE2018★ 5 cited

Ten Years of PAMELA in Space

O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +50

The PAMELA cosmic ray detector was launched on June 15th 2006 on board the Russian Resurs-DK1 satellite, and during ten years of nearly continuous data-taking it has observed new i…

physics.space-ph2018★ 11 cited

Unexpected cyclic behavior in cosmic ray protons observed by PAMELA at 1 AU

O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +50

Protons detected by the PAMELA experiment in the period 2006-2014 have been analyzed in the energy range between 0.40-50 GV to explore possible periodicities besides the well known…

physics.space-ph2018★ 89 cited

Proton fluxes measured by the PAMELA experiment from the minimum to the maximum solar activity for the 24th solar cycle

M. Martucci, R. Munini, M. Boezio +51

Precise measurements of the time-dependent intensity of the low energy ( GeV) galactic cosmic rays are fundamental to test and improve the models which describe their propagat…

astro-ph.HE2016★ 65 cited

Time dependence of the electron and positron components of the cosmic radiation measured by the PAMELA experiment between July 2006 and December 2015

O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +52

Cosmic-ray electrons and positrons are a unique probe of the propagation of cosmic rays as well as of the nature and distribution of particle sources in our Galaxy. Recent measurem…

physics.space-ph2016★ 34 cited

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…

physics.space-ph2016★ 2 cited

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…

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.HE2013★ 308 cited

The cosmic-ray positron energy spectrum measured by PAMELA

PAMELA Collaboration, O. Adriani, G. C. Barbarino +63

Precision measurements of the positron component in the cosmic radiation provide important information about the propagation of cosmic rays and the nature of particle sources in ou…

astro-ph.HE2013

Cosmic-Ray Positron Identification with the PAMELA experiment

O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +63

The PAMELA satellite borne experiment is designed to study cosmic rays with great accuracy in a wide energy range. One of PAMELA's main goal is the study of the antimatter componen…