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Optical technologies in ESA programmes - Congrex

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OPTICS:<br />

1.<br />

<strong>ESA</strong> has selected the Silicon Pore Optics as the<br />

basel<strong>in</strong>e mirror technology <strong>in</strong> its IXO development plan<br />

for 2008-2012 (req. HEW < 5 arcsec at 1.25 keV).<br />

2. Encourag<strong>in</strong>g results from Silicon Pore X-ray Optics:<br />

S<strong>in</strong>gle reflection HEW = 7 arcsec obta<strong>in</strong>ed from stack of 10<br />

plates (out of 45).<br />

CRYO-CHAIN:<br />

1. Maxi compressor (advanced l<strong>in</strong>ear compressor for e.g.<br />

10K cooler) TRP activity is runn<strong>in</strong>g with Astrium & RAL<br />

s<strong>in</strong>ce 2 years, 1 more year to go.<br />

2. 10K Stirl<strong>in</strong>g cooler (l<strong>in</strong>ked to previous activity) is runn<strong>in</strong>g<br />

with Astrium & RAL s<strong>in</strong>ce 2 years, 1 year to go.<br />

3.<br />

IXO technology - <strong>ESA</strong> funded<br />

The 50mK cooler development activity with CEA to<br />

develop sorption/ADR cooler comb<strong>in</strong>ation is runn<strong>in</strong>g s<strong>in</strong>ce<br />

Jan 2008 for a 24 months duration.<br />

Optics <strong>in</strong> <strong>ESA</strong> <strong>programmes</strong> | Roland Meynart | ICSO �ό��� 2010 | 05 October 2010 | Earth Observation | Slide 28

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