Precision Measurement of the Flux in Primary Cosmic Rays from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space Station
… We present a measurement of the cosmic ray (e + + e −) flux in the range 0.5 GeV to 1 TeV
based … In conclusion, the precision measurement of Φ(e + + e −) as a function of energy from …
based … In conclusion, the precision measurement of Φ(e + + e −) as a function of energy from …
Measurement of the cosmic Flux from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer (AMS-02) on the International Space Station
V Vagelli - 2014 - cds.cern.ch
… in May 2011 and that is collecting cosmic rays in the GeV to TeV energy range with no major
… The precise measurement of the cosmic et component represents one of the primary AMS …
… The precise measurement of the cosmic et component represents one of the primary AMS …
Measurement of the cosmic ray hadron spectrum up to 30 TeV at mountain altitude: the primary proton spectrum
M Aglietta, B Alessandro, P Antonioli, F Arneodo… - Astroparticle …, 2003 - Elsevier
… 2 s −1 sr −1 GeV −1 overthe energy range 30 GeV–30 TeV. The … Over a wide energy range
E 0 =0.5–50 TeV its best fit is … A precise knowledge of such spectra is of particular importance …
E 0 =0.5–50 TeV its best fit is … A precise knowledge of such spectra is of particular importance …
… Alpha Magnetic Spectrometer on the International Space Station:<? format?> Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–350 GeV
…, H Esser, A Falvard, E Fiandrini, A Fiasson, E Finch… - Physical Review Letters, 2013 - APS
… 10–180 GeV=c charged pions which produce transition radiation as protons up to 1:2 TeV=c…
and the sides, to simulate the arrival of cosmic rays at AMS on the ISS. These data have a …
and the sides, to simulate the arrival of cosmic rays at AMS on the ISS. These data have a …
Precision Measurement of the (e+ + e[superscript −) Flux in Primary Cosmic Rays from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer on the International …
… We present a measurement of the cosmic ray (e + + e −) flux in the range 0.5 GeV to 1 TeV
based … In conclusion, the precision measurement of Φ(e + + e −) as a function of energy from …
based … In conclusion, the precision measurement of Φ(e + + e −) as a function of energy from …
[HTML][HTML] 'Excess' of primary cosmic ray electrons
X Li, ZQ Shen, BQ Lu, TK Dong, YZ Fan, L Feng… - Physics Letters B, 2015 - Elsevier
… With the accurate cosmic ray (CR) electron and positron … ϵ e > 20 GeV where the solar
modulation of cosmic ray fluxes is … at energies of 100 GeV, 400 GeV and 1 TeV, respectively. We …
modulation of cosmic ray fluxes is … at energies of 100 GeV, 400 GeV and 1 TeV, respectively. We …
Electron and positron fluxes in primary cosmic rays measured with the Alpha Magnetic Spectrometer on the International Space Station
… Precision measurements by the Alpha Magnetic Spectrometer on the International Space
Station of the primary cosmic-ray electron flux in the range 0.5 to 700 GeV … to the TeV region (…
Station of the primary cosmic-ray electron flux in the range 0.5 to 700 GeV … to the TeV region (…
Observation of the anisotropy of 10 TeV primary cosmic ray nuclei flux<? format?> with the Super-Kamiokande-I detector
… energy is about 10 times larger [10], while the spread in the primary cosmic ray energy is …
, sensitive to primary cosmic rays with energy in the range several TeV to several hundred TeV. …
, sensitive to primary cosmic rays with energy in the range several TeV to several hundred TeV. …
[PDF][PDF] Towards Understanding the Origin of Cosmic-Ray Electrons
AMS Collaboration… - … LETTERS Phys Rev …, 2019 - pdfs.semanticscholar.org
… In conclusion, we have presented the high statistics precision measurements of the electron
flux from 0.5 GeV to 1.4 TeV, with detailed study of systematic uncertainties based on a data …
flux from 0.5 GeV to 1.4 TeV, with detailed study of systematic uncertainties based on a data …
A New Measurement of the Intensities of the Heavy Primary Cosmic-Ray Nuclei around 1 TeV amu–1
F Gahbauer, G Hermann, JR Hörandel… - The Astrophysical …, 2004 - iopscience.iop.org
… -ray nuclei O, Ne, Mg, Si, and Fe from 10 GeV amuÀ1 to … are 0.5 cm thick and are divided
into four quadrants of 1 m2 area … Accurate trajectory information is needed to correct for spatial …
into four quadrants of 1 m2 area … Accurate trajectory information is needed to correct for spatial …