The Alpha Magnetic Spectrometer (AMS) on the international space station: Part II—Results from the first seven years
M Aguilar, LA Cavasonza, G Ambrosi, L Arruda, N Attig… - Physics reports, 2021 - Elsevier
Abstract The Alpha Magnetic Spectrometer (AMS) is a precision particle physics detector on
the International Space Station (ISS) conducting a unique, long-duration mission of …
the International Space Station (ISS) conducting a unique, long-duration mission of …
Theory of cosmic ray transport in the heliosphere
Modelling the transport of cosmic rays (CRs) in the heliosphere represents a global
challenge in the field of heliophysics, in that such a study, if it were to be performed from first …
challenge in the field of heliophysics, in that such a study, if it were to be performed from first …
Review of particle physics
Particle Data Group, RL Workman… - … of theoretical and …, 2022 - academic.oup.com
The Review summarizes much of particle physics and cosmology. Using data from previous
editions, plus 2,143 new measurements from 709 papers, we list, evaluate, and average …
editions, plus 2,143 new measurements from 709 papers, we list, evaluate, and average …
Precision measurement of the proton flux in primary cosmic rays from rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station
M Aguilar, D Aisa, B Alpat, A Alvino, G Ambrosi… - Physical review …, 2015 - APS
A precise measurement of the proton flux in primary cosmic rays with rigidity
(momentum/charge) from 1 GV to 1.8 TV is presented based on 300 million events …
(momentum/charge) from 1 GV to 1.8 TV is presented based on 300 million events …
Galactic cosmic rays in the local interstellar medium: Voyager 1 observations and model results
AC Cummings, EC Stone, BC Heikkila… - The Astrophysical …, 2016 - iopscience.iop.org
ABSTRACT Since 2012 August Voyager 1 has been observing the local interstellar energy
spectra of Galactic cosmic-ray nuclei down to 3 MeV nuc− 1 and electrons down to 2.7 MeV …
spectra of Galactic cosmic-ray nuclei down to 3 MeV nuc− 1 and electrons down to 2.7 MeV …
Precision measurement of the helium flux in primary cosmic rays of rigidities 1.9 GV to 3 TV with the alpha magnetic spectrometer on the international space station
M Aguilar, D Aisa, B Alpat, A Alvino, G Ambrosi… - Physical review …, 2015 - APS
Knowledge of the precise rigidity dependence of the helium flux is important in
understanding the origin, acceleration, and propagation of cosmic rays. A precise …
understanding the origin, acceleration, and propagation of cosmic rays. A precise …
Development of the model of galactic interstellar emission for standard point-source analysis of Fermi Large Area Telescope data
F Acero, M Ackermann, M Ajello, A Albert… - The Astrophysical …, 2016 - iopscience.iop.org
Most of the celestial γ rays detected by the Large Area Telescope (LAT) on board the Fermi
Gamma-ray Space Telescope originate from the interstellar medium when energetic cosmic …
Gamma-ray Space Telescope originate from the interstellar medium when energetic cosmic …
Observation of the identical rigidity dependence of He, C, and O cosmic rays at high rigidities by the alpha magnetic spectrometer on the international space station
M Aguilar, L Ali Cavasonza, B Alpat, G Ambrosi… - Physical review …, 2017 - APS
We report the observation of new properties of primary cosmic rays He, C, and O measured
in the rigidity (momentum/charge) range 2 GV to 3 TV with 90× 10 6 helium, 8.4× 10 6 …
in the rigidity (momentum/charge) range 2 GV to 3 TV with 90× 10 6 helium, 8.4× 10 6 …
Cosmic ray measurements from Voyager 2 as it crossed into interstellar space
EC Stone, AC Cummings, BC Heikkila, N Lal - Nature Astronomy, 2019 - nature.com
The interaction of the interstellar and solar winds is complex, as revealed by differences in
intensities and anisotropies of low-energy ions (> 0.5 MeV per nucleon) originating inside …
intensities and anisotropies of low-energy ions (> 0.5 MeV per nucleon) originating inside …
[HTML][HTML] Monte Carlo design studies for the Cherenkov telescope array
K Bernlöhr, A Barnacka, Y Becherini, OB Bigas… - Astroparticle …, 2013 - Elsevier
The Cherenkov Telescopes Array (CTA) is planned as the future instrument for very-high-
energy (VHE) gamma-ray astronomy with a wide energy range of four orders of magnitude …
energy (VHE) gamma-ray astronomy with a wide energy range of four orders of magnitude …