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Proceedings Paper

Maximum-energy Auger-shower satellite (MASS/AIRWATCH)
Author(s): Yoshiyuki Takahashi; Russell A. Chipman; John O. Dimmock; Lloyd W. Hillman; David J. Lamb; Thomas M. Leslie; Jeffrey J. Weimer; Mark J. Christl; Gerald J. Fishman; Thomas A. Parnell; Louis M. Barbier; Kevin R. Boyce; Eric R. Christian; John F. Krizmanic; John W. Mitchell; Jonathan F. Ormes; Floyd W. Stecker; Donald E. Stilwell; Robert E. Streitmatter; Eugene C. Loh; Pierre Sokolski; Paul Sommers; Michael L. Cherry; John Linsley; Livio Scarsi
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Paper Abstract

A concept for observation from space of the highest energy cosmic rays above 1020 eV with a satellite-borne observatory has been considered. A maximum-energy auger (air)-shower satellite (MASS) would use segmented lenses (and/or mirrors) and an array of imaging devices (about 106 pixels) to detect and record fluorescent light profiles of cosmic ray cascades in the atmosphere. The field-of-view of MASS could be extended to about (1000 km)2 so that more than 103 events per year could be observed above 1020 eV. From far above the atmosphere, MASS would be capable of observing events at all angles including near horizontal tracks, and would have considerable aperture for high energy photon and neutrino observation. With a large aperture and the spatial and temporal resolution, MASS could determine the energy spectrum, the mass composition, and arrival anisotropy of cosmic rays from 1020 eV to 1022 eV, a region hitherto not explored by ground-based detectors such as the fly's eye and air-shower arrays. MASS's ability to identify comic neutrinos and gamma rays may help providing evidence for the theory which attributes the above cut-off cosmic ray flux to the decay of topological defects.

Paper Details

Date Published: 18 October 1996
PDF: 11 pages
Proc. SPIE 2806, Gamma-Ray and Cosmic-Ray Detectors, Techniques, and Missions, (18 October 1996); doi: 10.1117/12.253970
Show Author Affiliations
Yoshiyuki Takahashi, Univ. of Alabama in Huntsville (United States)
Russell A. Chipman, Univ. of Alabama in Huntsville (United States)
John O. Dimmock, Univ. of Alabama in Huntsville (United States)
Lloyd W. Hillman, Univ. of Alabama in Huntsville (United States)
David J. Lamb, Univ. of Alabama in Huntsville (United States)
Thomas M. Leslie, Univ. of Alabama in Huntsville (United States)
Jeffrey J. Weimer, Univ. of Alabama in Huntsville (United States)
Mark J. Christl, NASA Marshall Space Flight Ctr. (United States)
Gerald J. Fishman, NASA Marshall Space Flight Ctr. (United States)
Thomas A. Parnell, NASA Marshall Space Flight Ctr. (United States)
Louis M. Barbier, NASA Goddard Space Flight Ctr. (United States)
Kevin R. Boyce, NASA Goddard Space Flight Ctr. (United States)
Eric R. Christian, NASA Goddard Space Flight Ctr. (United States)
John F. Krizmanic, NASA Goddard Space Flight Ctr. (United States)
John W. Mitchell, NASA Goddard Space Flight Ctr. (United States)
Jonathan F. Ormes, NASA Goddard Space Flight Ctr. (United States)
Floyd W. Stecker, NASA Goddard Space Flight Ctr. (United States)
Donald E. Stilwell, NASA Goddard Space Flight Ctr. (United States)
Robert E. Streitmatter, NASA Goddard Space Flight Ctr. (United States)
Eugene C. Loh, Univ. of Utah (United States)
Pierre Sokolski, Univ. of Utah (United States)
Paul Sommers, Univ. of Utah (United States)
Michael L. Cherry, Louisiana State Univ. (United States)
John Linsley, Univ. of New Mexico (Italy)
Livio Scarsi, Istituto Fisica Cosmica e Applicazione Informatica (Italy)


Published in SPIE Proceedings Vol. 2806:
Gamma-Ray and Cosmic-Ray Detectors, Techniques, and Missions
Brian D. Ramsey; Thomas A. Parnell, Editor(s)

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