Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spie.6275e..11t&link_type=abstract
Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III. Edited by Zmuidzinas, Jonas; Holland, Wayne S.; W
Astronomy and Astrophysics
Astronomy
Scientific paper
We describe a miniature dilution refrigerator (MDR), operated in continuous mode and suitable for many detector applications at temperatures down to 50 mK. It distinguishes itself from other refrigerators in that it is self-contained and benefits from an internal cycle of the 3He gas. As a result, no external gas handling system is required so size, weight and complexity of the system is dramatically decreased. The system has no fine capillaries, moving parts or cooled O-rings. It is therefore mechanically very reliable, has no risk of blockages and is unlikely to develop cryogenic leaks. One direct application is balloon-borne or ground-based observations of the CMB using large detector arrays. When these experiments are operated remotely on platforms or at sites with limited infrastructure and maintenance support, a compact and reliable dilution refrigerator becomes essential. We describe a complete system incorporating an MDR which we have built and integrated with a pulse-tube refrigerator to achieve a cooling power of several micro Watt at 100 mK. This system is being developed for a CMB polarization experiment (CLOVER) which requires three independent cryostats to cool large TES detector arrays.
Chase Simon T.
Piccirillo Lucio
Teleberg Gustav
No associations
LandOfFree
A miniature dilution refrigerator for sub-Kelvin detector arrays does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A miniature dilution refrigerator for sub-Kelvin detector arrays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A miniature dilution refrigerator for sub-Kelvin detector arrays will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1893648