Hayton, Darren, Hargrave, Peter Charles ![]() |
Abstract
We present details of a new illumination source, suitable for use on mid-infrared satellite instruments. The device is based around an electrically heated tungsten filament. The source is compact, and dissipates typically 9 mW for an effective black-body temperature of 1000 K. A typical device design will warm from 4 K to 1000 K in around 1 s, and cool from 1000 K to 4 K in around 2.5 s. We present results for a range of device designs, and discuss the range of parameter space (e.g. power dissipation, time constant, photon flux) to which these devices can be tuned. A device of this type is currently in qualification for flight on JWST-MIRI1, and similar devices are being considered for use on JWST-NIRSPEC and SPICA2-ESI3.
Item Type: | Conference or Workshop Item (Paper) |
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Date Type: | Publication |
Status: | Published |
Schools: | Schools > Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Publisher: | SPIE |
ISBN: | 9780819463302 |
ISSN: | 0277786X |
Related URLs: | |
Last Modified: | 25 Oct 2022 09:38 |
URI: | https://orca.cardiff.ac.uk/id/eprint/59444 |
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