The atmospheric X-ray imaging spectrometer (AXIS) instrument: Quantifying energetic particle precipitation through bremsstrahlung X-ray imaging

Author:

Berland G. D.1ORCID,Marshall R. A.1ORCID,Martin C.1,Buescher J.1,Kohnert R. A.2ORCID,Boyajian S.2,Cully C. M.3ORCID,McCarthy M. P.4ORCID,Xu W.1

Affiliation:

1. Aerospace Engineering Sciences, University of Colorado Boulder 1 , Boulder, Colorado 80303, USA

2. Laboratory of Atmospheric and Space Physics (LASP) at the University of Colorado Boulder 2 , Boulder, Colorado 80303, USA

3. Department of Physics & Astronomy, University of Calgary 3 , Calgary, Alberta T2N 1N4, Canada

4. Department of Earth and Space Sciences, University of Washington Seattle 4 , Seattle, Washington 98195, USA

Abstract

The Atmospheric X-ray Imaging Spectrometer (AXIS) described in this work is a compact, wide field-of-view, hard x-ray imager. The AXIS instrument will fly onboard the Atmospheric Effects of Precipitation through Energetic X-rays (AEPEX) 6U CubeSat mission and will measure bremsstrahlung x-ray photons in the 50–240 keV range with cadmium–zinc–telluride (CZT) detectors using coded aperture optics. AXIS will measure photons generated by energetic particle precipitation for the purpose of determining the spatial scales of precipitation and estimating electron precipitation characteristics. This paper describes the design and testing of the AXIS instrument, including a summary of simulations performed that motivate the shielding, optics, and mechanical design. Testing and characterization is reported that validates the instrument design and shows that the instrument design meets or exceeds the measurement requirements necessary for AEPEX mission success.

Funder

Heliophysics Division

Publisher

AIP Publishing

Subject

Instrumentation

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