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SPIRE Design Description - Research Services

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Draft <strong>SPIRE</strong> <strong>Design</strong> <strong>Description</strong> Document<br />

Figure 4-39 - Simulated spectrum of the 80 K telescope seen through the <strong>SPIRE</strong> FTS with representation optical<br />

filtering. The black line is before applying the frequency response of the detectors the red line after. Note the much<br />

larger rate of change of the sign<br />

4.10 FPU structure<br />

Parameter Specification<br />

L1<br />

Heat leak to FPU from FIRST Optical Bench<br />

L0<br />

Conductive heat leaks down 2K box supports<br />

300mK<br />

Parasitic heat leak on 300mK detector stage<br />

300mK<br />

Heat leak down the Photometer 300mK strap supports<br />

300mK<br />

Heat leak down the Spectrometer 300mK strap supports<br />

The structure has three main requirements:<br />

1. To mechanically support and positively locate the components (optical or otherwise) of the<br />

photometer and the spectrometer;<br />

2. To provide the correct thermal isolation between the various temperature stages of the instrument;<br />

and<br />

98<br />

6mW<br />

(for ∆T = 11-4.2 = 6.8K)<br />

1mW<br />

(for ∆T = 4.2 - 1.7 = 2.5K)<br />

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