Indications of proton-dominated cosmic-ray composition above 1.6 EeV.

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Bibliographic Details
Title: Indications of proton-dominated cosmic-ray composition above 1.6 EeV.
Authors: Abbasi RU; Department of Physics, University of Utah, Salt Lake City, Utah, USA., Abu-Zayyad T, Al-Seady M, Allen M, Amman JF, Anderson RJ, Archbold G, Belov K, Belz JW, Bergman DR, Blake SA, Brusova OA, Burt GW, Cannon C, Cao Z, Deng W, Fedorova Y, Finley CB, Gray RC, Hanlon WF, Hoffman CM, Holzscheiter MH, Ivanov D, Hughes G, Hüntemeyer P, Ivanov D, Jones BF, Jui CC, Kim K, Kirn MA, Loh EC, Liu J, Lundquist JP, Maestas MM, Manago N, Marek LJ, Martens K, Matthews JA, Matthews JN, Moore SA, O'Neill A, Painter CA, Perera L, Reil K, Riehle R, Roberts M, Rodriguez D, Sasaki N, Schnetzer SR, Scott LM, Sinnis G, Smith JD, Sokolsky P, Song C, Springer RW, Stokes BT, Stratton S, Thomas SB, Thomas JR, Thomson GB, Tupa D, Zech A, Zhang X
Corporate Authors: High Resolution Fly's Eye Collaboration
Source: Physical review letters [Phys Rev Lett] 2010 Apr 23; Vol. 104 (16), pp. 161101. Date of Electronic Publication: 2010 Apr 20.
Publication Type: Journal Article
Journal Info: Publisher: American Physical Society Country of Publication: United States NLM ID: 0401141 Publication Model: Print-Electronic Cited Medium: Internet ISSN: 1079-7114 (Electronic) Linking ISSN: 00319007 NLM ISO Abbreviation: Phys Rev Lett Subsets: PubMed not MEDLINE
Database: MEDLINE Ultimate
Description
ISSN:1079-7114
DOI:10.1103/PhysRevLett.104.161101