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 …

Materials challenges for the Starshot lightsail

HA Atwater, AR Davoyan, O Ilic, D Jariwala… - Nature materials, 2018 - nature.com
The Starshot Breakthrough Initiative established in 2016 sets an audacious goal of sending
a spacecraft beyond our Solar System to a neighbouring star within the next half-century. Its …

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 …

PAMELA measurements of cosmic-ray proton and helium spectra

O Adriani, GC Barbarino, GA Bazilevskaya, R Bellotti… - Science, 2011 - science.org
Protons and helium nuclei are the most abundant components of the cosmic radiation.
Precise measurements of their fluxes are needed to understand the acceleration and …

Atmospheric neutrino flux calculation using the NRLMSISE-00 atmospheric model

M Honda, MS Athar, T Kajita, K Kasahara… - Physical Review D, 2015 - APS
We extend our calculation of the atmospheric neutrino fluxes to polar and tropical regions. It
is well known that the air density profiles in the polar and the tropical regions are different …

The Relativistic Electron-Proton Telescope (REPT) instrument on board the Radiation Belt Storm Probes (RBSP) spacecraft: Characterization of Earth's radiation belt …

DN Baker, SG Kanekal, VC Hoxie, S Batiste… - The van allen probes …, 2014 - Springer
Particle acceleration and loss in the million electron Volt (MeV) energy range (and above) is
the least understood aspect of radiation belt science. In order to measure cleanly and …

[PDF][PDF] The FLUKA code: Description and benchmarking

G Battistoni, F Cerutti, A Fasso, A Ferrari… - AIP Conference …, 2007 - fluka.org
The FLUKA code: description and benchmarking Page 1 The FLUKA code: description and
benchmarking G. Battistoni*, F. Cerutti^ A. Fasso**, A. Ferrari1', S. Muraro*, J. Ranft*, S. Roesle …

Measurement of atmospheric neutrino oscillation parameters by Super-Kamiokande I

Y Ashie, J Hosaka, K Ishihara, Y Itow, J Kameda… - Physical Review D …, 2005 - APS
We present a combined analysis of fully-contained, partially-contained and upward-going
muon atmospheric neutrino data from a 1489 d exposure of the Super-Kamiokande detector …

Calculation of atmospheric neutrino flux using the interaction model calibrated<? format?> with atmospheric muon data

M Honda, T Kajita, K Kasahara, S Midorikawa… - Physical Review D …, 2007 - APS
Using the “modified DPMJET-III” model explained in the previous paper [T. Sanuki,
preceding Article, Phys. Rev. D 75, 043005 (2007). PRVDAQ 0556-2821], we calculate the …

Energy spectra of abundant nuclei of primary cosmic rays from the data of ATIC-2 experiment: Final results

AD Panov, JH Adams, HS Ahn… - Bulletin of the Russian …, 2009 - Springer
The final results of processing the data from the balloon-born experiment ATIC-2 (Antarctica,
2002–2003) for the energy spectra of protons and He, C, O, Ne, Mg, Si, and Fe nuclei, the …