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260. Measurement of the Cosmic‐Ray Energy Spectrum and Composition from 1017to 1018.3eV Using a Hybrid Technique

268. Erratum: Evidence for Changing of Cosmic Ray Composition between1017and1018eVfrom Multicomponent Measurements [Phys. Rev. Lett. 84, 4276 (2000)]

271. Evidence for Changing of Cosmic Ray Composition between1017and1018eV from Multicomponent Measurements

278. Study of Broad‐Scale Anisotropy of Cosmic‐Ray Arrival Directions from \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $2\times 10^{17}$ \end{document} to 1020Electron Volts from Fly's Eye Data

279. Pulse Amplification and Shaping Using a Nonlinear Amplifying Loop Mirror

286. Atmospheric studies using the high-resolution fly's eye xenon flasher array

294. Detection of a cosmic ray with measured energy well beyond the expected spectral cutoff due to cosmic microwave radiation

297. Results from the fly’s eye experiment

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