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

308 citations · 1.8k across the 34 of their papers we have counts for

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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.SR2021★ 38 cited

New reconstruction of event-integrated spectra (spectral fluences) for major solar energetic particle events

Sergey A. Koldobskiy, Osku Raukunen, Rami Vainio +2

Fluences of solar energetic particles (SEPs) are not easy to evaluate, especially for high-energy events (i.e. ground-level enhancements, GLEs). Earlier estimates of event-integrat…

astro-ph.SR2020★ 50 cited

Revisited reference solar proton event of 23-Feb-1956: Assessment of the cosmogenic-isotope method sensitivity to extreme solar events

Ilya G. Usoskin, Sergey A. Koldobskiy, Gennady A. Kovaltsov +4

Our direct knowledge of solar eruptive events is limited to several decades and does not include extreme events, which can only be studied by the indirect proxy method over millenn…

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.SR2015★ 142 cited

Time dependence of the e^- flux measured by PAMELA during the July 2006 - December 2009 solar minimum

O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +58

Precision measurements of the electron component in the cosmic radiation provide important information about the origin and propagation of cosmic rays in the Galaxy not accessible…

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…