Modelling the path length of aluminium seen by the detectors in the MIRI instrument on the JWST

A. C. H. Glasse; D. Lee; P. Samara-Ratna; G. H. Rieke

doi:10.1117/12.2561035

13 December 2020 Modelling the path length of aluminium seen by the detectors in the MIRI instrument on the JWST

A. C. H. Glasse, D. Lee, P. Samara-Ratna, G. H. Rieke

Proceedings Volume 11443, Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave; 114434D (2020) https://doi.org/10.1117/12.2561035
Event: SPIE Astronomical Telescopes + Instrumentation, 2020, Online Only

Conference Poster

Abstract

The MIRI instrument on the James Webb Space Telescope is equipped with detectors which are susceptible to signal disruption by the charge deposited from impacting cosmic rays. In order to quantify the degree to which the structure of MIRI will shield the detectors, we have used an opto-mechanical ray tracing approach, whereby the solid bodies in a detailed 3D model of the instrument are substituted with an absorptive glassy material. By importing this modified model into a ray tracing program (Tracepro) and then launching many rays from the detector, we have been able to generate a map of aluminium path length as a function of direction. We find that there is a minimum thickness of 2 to 3 mm over a few patches which subtend no more than 1.5 % of the sky for the worst case, imager detector. We discuss the performance of the shielding provided by the MIRI structure, concluding that this minimum thickness of aluminium is sufficient to suppress the impact of low energy protons below the level of the unavoidable flux due to high energy cosmic rays.

Citation Download Citation

A. C. H. Glasse, D. Lee, P. Samara-Ratna, and G. H. Rieke "Modelling the path length of aluminium seen by the detectors in the MIRI instrument on the JWST", Proc. SPIE 11443, Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave, 114434D (13 December 2020); https://doi.org/10.1117/12.2561035

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