The Alpha Magnetic Spectrometer (AMS)on the International Space Station : Part I - results from the test flight on the space shuttle
By M. Aguilar, J. Alcaraz, J. Allaby, B. Alpat, G. Ambrosi, H. Anderhub, L. Ao, A. Arefiev, P. Azzarello, E. Babucci and 209 more. 2002
395 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/1bec93602ff0603686853e0ee640a77928e06637
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Citations in the corpus
- COSMIC-RAY PROTON AND HELIUM SPECTRA FROM THE FIRST CREAM FLIGHT (2011, background): “Likewise, the CREAM helium spectrum is harder than AMS, 2.740 ± 0.01 at 20−200 GV and BESS, 2.699 ± 0.040 from 20 GeV nucleon−1 to a few hundred GeV nucleon−1.”
- THE LARGE AREA TELESCOPE ON THE FERMI GAMMA-RAY SPACE TELESCOPE MISSION (2009, methodology): “For albedo fluxes of particles with energies below∼150 MeV, inaccessible to the AMS and other large instruments, measurements made by NINA and NINA-2 and a series of Russian satellite experiments with an instrument known as Mariya are used.”
- History of dark matter (2018, neutral): “…of time, great progress has also been made in the measurement of the cosmic-ray antiproton spectrum, including successive advances by the CAPRICE (Boezio et al., 1997, 2001), BESS (Asaoka et al., 2002; Abe et al., 2008), AMS-01 (Aguilar et al., 2002), and PAMELA (Adriani et al., 2010) experiments.”
- DISCREPANT HARDENING OBSERVED IN COSMIC-RAY ELEMENTAL SPECTRA (2010, background): “The latter have provided primary cosmic-ray energy spectra with rather good precision at energies up to ~10 11 eV/nucleon (e.g., Engelmann et al. 1990; Müller et al. 1991; Aguilar et al. 2002; Haino et al. 2004).”