154 citations · 609 across the 18 of their papers we have counts for
13 papers · 1 filter
Spectra of He isotopes and the He/He ratio
M. J. Boschini, S. Della Torre, M. Gervasi +11
Since its launch, the Alpha Magnetic Spectrometer-02 (AMS-02) has delivered outstanding quality measurements of the spectra of cosmic-ray (CR) species, , , and nu…
Spectra of Cosmic Ray Sodium and Aluminum and Unexpected Aluminum Excess
M. J. Boschini, S. Della Torre, M. Gervasi +11
Since its launch, the Alpha Magnetic Spectrometer-02 (AMS-02) has delivered outstanding quality measurements of the spectra of cosmic-ray (CR) species, , , and nu…
A Hint of a Low-Energy Excess in Cosmic-Ray Fluorine
M. J. Boschini, S. Della Torre, M. Gervasi +11
Since its launch, the Alpha Magnetic Spectrometer-02 (AMS-02) has delivered outstanding quality measurements of the spectra of cosmic-ray (CR) species, , , and nu…
A discovery of a low-energy excess in cosmic-ray iron: an evidence of the past supernova activity in the Local Bubble
M. J. Boschini, S. Della Torre, M. Gervasi +11
Since its launch, the Alpha Magnetic Spectrometer - 02 (AMS-02) has delivered outstanding quality measurements of the spectra of cosmic-ray (CR) species, , , and…
Inference of the Local Interstellar Spectra of Cosmic Ray Nuclei Z<=28 with the GalProp-HelMod Framework
M. J. Boschini, S. Della Torre, M. Gervasi +11
Composition and spectra of Galactic cosmic rays (CRs) are vital for studies of high-energy processes in a variety of environments and on different scales, for interpretation of gam…
Deciphering the local Interstellar spectra of secondary nuclei with GALPROP/HelMod framework and a hint for primary lithium in cosmic rays
M. J. Boschini, S. Della Torre, M. Gervasi +11
Local interstellar spectra (LIS) of secondary cosmic ray (CR) nuclei, lithium, beryllium, boron, and partially secondary nitrogen, are derived in the rigidity range from 10 MV to ~…
Deciphering the local Interstellar spectra of primary cosmic ray species with HelMod
M. J. Boschini, S. Della Torre, M. Gervasi +11
Local interstellar spectra (LIS) of primary cosmic ray (CR) nuclei, such as helium, oxygen, and mostly primary carbon are derived for the rigidity range from 10 MV to ~200 TV using…
HelMod in the works: from direct observations to the local interstellar spectrum of cosmic-ray electrons
M. J. Boschini, S. Della Torre, M. Gervasi +11
The local interstellar spectrum (LIS) of cosmic-ray (CR) electrons for the energy range 1 MeV to 1 TeV is derived using the most recent experimental results combined with the state…
Solution of heliospheric propagation: unveiling the local interstellar spectra of cosmic ray species
M. J. Boschini, S. Della Torre, M. Gervasi +14
Local interstellar spectra (LIS) for protons, helium and antiprotons are built using the most recent experimental results combined with the state-of-the-art models for propagation…
Precision measurement of the (e + e) flux in primary cosmic rays from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space Station
Manuela Vecchi
We present a precise measurement of the combined electron plus positron flux from 0.5 GeV to 1 TeV, based on the analysis of the data collected by the Alpha Magnetic Spectrometer d…
From Observations near the Earth to the Local Interstellar Spectra
S. Della Torre, M. Gervasi, D. Grandi +9
Propagation of cosmic rays (CRs) from their sources to the observer is described mainly as plain diffusion at high energies, while at lower energies there are other physical proces…
Precision Measurement of the Proton Flux in Primary Cosmic Rays from 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station
Cristina Consolandi
A precision measurement of the proton flux in primary cosmic rays with rigidity from 1 GV to 1.8 TV is presented based on 300 million events. The results show that the proton flux…
HelMod: A Comprehensive Treatment of the Cosmic Ray Transport Through the Heliosphere
S. Della Torre, M. Gervasi, D. Grandi +9
HelMod is a code evaluating the transport of Galactic cosmic rays through the inner heliosphere down to Earth. It is based on a 2-D Monte Carlo approach and includes a general desc…