Cosmic-ray spectra of primary protons and high altitude muons deconvolved from observed atmospheric gamma rays
Author:
Publisher
American Physical Society (APS)
Subject
Nuclear and High Energy Physics
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.74.083511/fulltext
Reference39 articles.
1. Measurements of the Solar Neutrino Flux from Super-Kamiokande's First 300 Days
2. Emulsion chamber observations of primary cosmic-ray electrons in the energy range 30-1000 GeV
3. Atmospheric gamma-ray observation with the BETS detector for calibrating atmospheric neutrino flux calculations
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1. Directional sensitivity of MuSTAnG muon telescope;Journal of Space Weather and Space Climate;2013
2. OBSERVATIONS OF HIGH-ENERGY COSMIC-RAY ELECTRONS FROM 30 GeV TO 3 TeV WITH EMULSION CHAMBERS;The Astrophysical Journal;2012-11-16
3. Atmospheric electron spectrum above 30GeV at the high altitude;Astroparticle Physics;2012-10
4. Cosmic ray primary composition in the energy range 10–1000 TeV obtained by passive balloon-borne detector: Reanalysis of the RUNJOB experiment;Physical Review D;2009-04-30
5. Cosmic-ray electron spectrum above 100GeV from PPB-BETS experiment in Antarctica;Advances in Space Research;2008-11
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