DSRI has initiated a development program of CZT X-ray and gamma-ray detecto
rs employing strip readout techniques. A dramatic improvement of the energy
response was found operating the detectors as the so-called drift detector
s. For the electronic readout, modern ASIC chips were investigated. Modular
design and the low-power electronics will make large area detectors using
the drift strip method feasible. The performance of a prototype CZT system
will be presented and discussed. One such detector system has been proposed
for future space missions: the X-Ray Imager (XRI) on the Atmospheric X-ray
Observatory (AXO), which is a mission proposed to the Danish Small Satelli
te Program and is dedicated to observations of X-ray generating processes i
n the Earth's atmosphere. Of special interest will be simultaneous optical
and X-ray observations of sprites that are flashes appearing directly above
an active thunderstorm system. Additional objective is a detailed mapping
of the auroral X-ray and optical emission. XRI comprises a coded mask and a
20 x 40cm(2) CZT detector array covering an energy range from 5 to 200keV.
(C) 2001 Elsevier Science B.V. All rights reserved.