Ultra-Heavy Galactic Cosmic Ray Elemental Abundances and the ACCESS Mission

Details Ultra-Heavy Galactic Cosmic Ray Elemental Abundances and the ACCESS Mission Ultra-Heavy Galactic Cosmic Ray Elemental Abundances and the ACCESS Mission

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aps..apr..d310b&link_type=abstract

American Physical Society, APS/AAPT Joint April Meeting, April 18-21, 1998 Columbus, Ohio, abstract #D3.10

Physics

Scientific paper

The Advanced Cosmic Ray Composition Experiment for Space Station (ACCESS) has been approved by NASA for a mission concept study. There are three modules which constitute the ACCESS experiment in its present concept. In this paper we will discuss the UH-module which has been selected for an instrument definition study. The primary objective of the UH module is the measurement of all elemental abundances over the charge range from iron through uranium. We will discuss the science objectives and the instrument technique which we are currently developing.

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