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Thermodynamic Performance of the 3-Stage ADR for the Astro-H Soft X-Ray Spectrometer Instrument

Authors :
Peter J Shirron
Mark O Kimball
Bryan L James
Theodore Muench
Michael J DiPirro
Thomas G Bialas
Gary A Sneiderman
Frederick S Porter
Richard L Kelley
Source :
Cryogenics. 74
Publication Year :
2015
Publisher :
United States: NASA Center for Aerospace Information (CASI), 2015.

Abstract

The Soft X-ray Spectrometer (SXS) instrument[1] on Astro-H[2] will use a 3-stage ADR[3] to cool the microcalorimeter array to 50 mK. In the primary operating mode, two stages of the ADR cool the detectors using superfluid helium at ≤1.20 K as the heat sink[4]. In the secondary mode, which is activated when the liquid helium is depleted, the ADR uses a 4.5 K Joule-Thomson cooler as its heat sink. In this mode, all three stages operate together to continuously cool the (empty) helium tank and singleshot cool the detectors. The flight instrument - dewar, ADR, detectors and electronics - were integrated in 2014 and have since undergone extensive performance testing. This paper presents a thermodynamic analysis of the ADR's operation, including cooling capacity, heat rejection to the heat sinks, and various measures of efficiency.

Details

Language :
English
ISSN :
00112275
Volume :
74
Database :
NASA Technical Reports
Journal :
Cryogenics
Notes :
WBS 063015.02.02.01
Publication Type :
Report
Accession number :
edsnas.20150022480
Document Type :
Report
Full Text :
https://doi.org/10.1016/j.cryogenics.2015.10.011