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Y Katayose

Showing results (51-60 of 63) with videos related to

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Physical Review Letters|January 6, 2023
Cosmic-Ray Boron Flux Measured from 8.4  GeV/n to 3.8  TeV/n with the Calorimetric Electron Telescope on the International Space StationO Adriani, Y Akaike, K Asano, et al.
Physical Review Letters|July 31, 2025
Precision Spectral Measurements of Chromium and Titanium from 10 to 250  GeV/n and Sub-Iron to Iron Ratio with the Calorimetric Electron Telescope on the International Space StationO Adriani, Y Akaike, K Asano, et al.
Physical Review Letters|June 9, 2023
Charge-Sign Dependent Cosmic-Ray Modulation Observed with the Calorimetric Electron Telescope on the International Space StationO Adriani, Y Akaike, K Asano, et al.
Physical Review Letters|February 6, 2018
Evaluation of the Interplanetary Magnetic Field Strength Using the Cosmic-Ray Shadow of the SunM Amenomori, X J Bi, D Chen, et al.
Physical Review Letters|January 8, 2021
Direct Measurement of the Cosmic-Ray Carbon and Oxygen Spectra from 10  GeV/n to 2.2  TeV/n with the Calorimetric Electron Telescope on the International Space StationO Adriani, Y Akaike, K Asano, et al.
Physical Review Letters|September 13, 2013
Probe of the solar magnetic field using the "cosmic-ray shadow" of the sunM Amenomori, X J Bi, D Chen, et al.
Science (New York, N.Y.)|October 21, 2006
Anisotropy and corotation of galactic cosmic raysM Amenomori, S Ayabe, X J Bi, et al.
Physical Review Letters|December 9, 2017
Energy Spectrum of Cosmic-Ray Electron and Positron from 10 GeV to 3 TeV Observed with the Calorimetric Electron Telescope on the International Space StationO Adriani, Y Akaike, K Asano, et al.
Physical Review Letters|May 31, 2019
Direct Measurement of the Cosmic-Ray Proton Spectrum from 50 GeV to 10 TeV with the Calorimetric Electron Telescope on the International Space StationO Adriani, Y Akaike, K Asano, et al.
Physical Review Letters|September 7, 2019
First Detection of Photons with Energy beyond 100 TeV from an Astrophysical SourceM Amenomori, Y W Bao, X J Bi, et al.
Pageof 7

Showing results (51-60 of 63) with videos related to

Sort By:
Pageof 7
Physical Review Letters|January 6, 2023
Cosmic-Ray Boron Flux Measured from 8.4  GeV/n to 3.8  TeV/n with the Calorimetric Electron Telescope on the International Space StationO Adriani, Y Akaike, K Asano, et al.
Physical Review Letters|July 31, 2025
Precision Spectral Measurements of Chromium and Titanium from 10 to 250  GeV/n and Sub-Iron to Iron Ratio with the Calorimetric Electron Telescope on the International Space StationO Adriani, Y Akaike, K Asano, et al.
Physical Review Letters|June 9, 2023
Charge-Sign Dependent Cosmic-Ray Modulation Observed with the Calorimetric Electron Telescope on the International Space StationO Adriani, Y Akaike, K Asano, et al.
Physical Review Letters|February 6, 2018
Evaluation of the Interplanetary Magnetic Field Strength Using the Cosmic-Ray Shadow of the SunM Amenomori, X J Bi, D Chen, et al.
Physical Review Letters|January 8, 2021
Direct Measurement of the Cosmic-Ray Carbon and Oxygen Spectra from 10  GeV/n to 2.2  TeV/n with the Calorimetric Electron Telescope on the International Space StationO Adriani, Y Akaike, K Asano, et al.
Physical Review Letters|September 13, 2013
Probe of the solar magnetic field using the "cosmic-ray shadow" of the sunM Amenomori, X J Bi, D Chen, et al.
Science (New York, N.Y.)|October 21, 2006
Anisotropy and corotation of galactic cosmic raysM Amenomori, S Ayabe, X J Bi, et al.
Physical Review Letters|December 9, 2017
Energy Spectrum of Cosmic-Ray Electron and Positron from 10 GeV to 3 TeV Observed with the Calorimetric Electron Telescope on the International Space StationO Adriani, Y Akaike, K Asano, et al.
Physical Review Letters|May 31, 2019
Direct Measurement of the Cosmic-Ray Proton Spectrum from 50 GeV to 10 TeV with the Calorimetric Electron Telescope on the International Space StationO Adriani, Y Akaike, K Asano, et al.
Physical Review Letters|September 7, 2019
First Detection of Photons with Energy beyond 100 TeV from an Astrophysical SourceM Amenomori, Y W Bao, X J Bi, et al.
Pageof 7