In-orbit performance prediction for Amon-Ra energy channel instrument

  • Seong, Se-Hyun (Space Optics Laboratory, Dept. of Astronomy and Space Science, Yonsei University) ;
  • Hong, Jin-Suk (Yongin R&D Center, Samsung Thales Co., Ltd.) ;
  • Ryu, Dong-Ok (Space Optics Laboratory, Dept. of Astronomy and Space Science, Yonsei University) ;
  • Kim, Sug-Whan (Space Optics Laboratory, Dept. of Astronomy and Space Science, Yonsei University)
  • Published : 2011.04.15

Abstract

In this report, we present in-orbit radiometric performance prediction for the Amon-Ra (Albedo Monitor and Radiometer) energy channel instrument. The Integrated Ray Tracing (IRT) computational technique uses the ray sets arriving at the Amon-Ra instrument aperture orbiting around the L1 halo orbit. Using this, the variation of flux arriving at the energy channel detector was obtained when the Amon-Ra instrument including the energy channel design observes the Sun and Earth alternately. The flux detectability was verified at the energy channel detector (LME-500-A, InfraTecTM). The detector time response and RMS signal voltage were then derived from the simulated flux variation results. The computation results demonstrate that the designed energy channel optical system satisfies the in-orbit detectability requirement. The technical details of energy channel instrument design, IRT model construction, radiative transfer simulation and output signal computation results are presented together with future development plan.

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