Paper
15 July 2010 Thermal and mechanical architecture for the SAFARI focal plane assembly
J. Martignac
Author Affiliations +
Abstract
The very challenging SPICA/SAFARI scientific goals imply to cool most detector solutions below 100 mK. This implies to find reliable solutions providing not only very efficient thermal insulation between the different temperature stages, but also keeping the stray light level well below the foreseen astronomical background (20 aW/pixel !). The main constraint is the available power budget (1-2μW); this value includes optical, electrical and parasitic power loads. This poster describes how the Herschel/PACS Bolometer Focal Plane thermo-mechanical design can be adapted to the new thermal and optical needs, while keeping a sufficiently stiff structure to withstand launch vibrations. We give the first results on the thermal and mechanical behaviour obtained with a prototype.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
J. Martignac "Thermal and mechanical architecture for the SAFARI focal plane assembly", Proc. SPIE 7741, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V, 77412R (15 July 2010); https://doi.org/10.1117/12.856712
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KEYWORDS
Staring arrays

Sensors

Picture Archiving and Communication System

Bolometers

Optical filters

Prototyping

Spectroscopy

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