The High-Resolution Fly's Eye (I-IiRes) is an observatory for the highest e
nergy cosmic rays. It detects the nitrogen fluorescence light induced by th
e passage of giant cosmic ray extensive air showers through the atmosphere.
A two-site prototype of the observatory was operated from September 1994 t
o November 1996. In this paper we describe the components of that detector,
and the procedures used to calibrate the detector and characterise the atm
osphere. Data collected by the HiRes prototype are being used for physics s
tudies, including an analysis of the cosmic ray mass composition in the ene
rgy range from 10(17) to 10(18) eV. (C) 2000 Elsevier Science B.V. All righ
ts reserved.