ASTRONOMY & SPACE
GREAT brought high-resolution far-infrared spectroscopy to the airborne SOFIA observatory. CRYOVAC manufactured its cryostats.
Why cryogenics matters Liquid-helium and liquid-nitrogen cooling supported sensitive receiver operation. The instrument paper describes its modular design and performance during early science flights.
Publications Context & publication summaries 01 S. Heyminck, U. U. Graf, R. Güsten, J. Stutzki, H. W. Hübers & P. Hartogh · 2012
GREAT: the SOFIA high-frequency heterodyne instrument Instrument architecture, receiver technology and in-flight commissioning results.
DOI 10.1051/0004-6361/201218811 · arXiv:1203.2845
Sources & references arxiv.org/html/1203.2845v1 arxiv.org/abs/1203.2845 doi.org/10.1051/0004-6361/201218811
ASTRONOMY & SPACE
MICADO is a near-infrared camera for the ELT, developed by an international consortium led by MPE. CRYOVAC built its cryostat.
Cold optics, faint signals The cryostat houses cold optics and detectors. Cooling suppresses the instrument’s own thermal emission; adaptive optics corrects atmospheric blurring before the image reaches the camera.
Publications Context & publication summaries 01 R. Davies et al. · 2016
MICADO: first light imager for the E-ELT An overview of observing modes, the optical concept and mechanisms inside the cryostat.
DOI 10.1117/12.2233047 · arXiv:1607.01954
02 J.-U. Pott et al. · 2018
The MICADO first light imager for ELT: its astrometric performance The astrometric design: measuring stellar positions precisely, with calibration and distortion control.
DOI 10.1117/12.2312069 · arXiv:1807.07402
03 R. Davies et al. · The MICADO Consortium · 2021
MICADO: The Multi-Adaptive Optics Camera for Deep Observations A readable introduction to the camera’s observing capabilities and the astronomy they enable.
DOI 10.18727/0722-6691/5217 · The Messenger 182, 17–21
Sources & references www.mpe.mpg.de/ir/micado www.mpe.mpg.de/8022687/picturegallery elt.eso.org/instrument/MICADO/ arxiv.org/abs/1607.01954 doi.org/10.1117/12.2233047 doi.org/10.1117/12.2312069 doi.eso.org/10.18727/0722-6691/5217 doi.org/10.18727/0722-6691/5217
ASTRONOMY & SPACE
ESO’s Extremely Large Telescope is being built on Cerro Armazones in Chile. Its 39-metre primary mirror collects visible and near-infrared light.
Inside MICADO, the ELT’s near-infrared camera. ESO/MICADO consortium/L. Calçada · CC BY 4.0 ESO engineering illustration · resized and converted to WebP. Image source & licence ESO ann24013d
From telescope to instrument The telescope gathers light; instruments such as MICADO turn it into scientific images and spectra. Adaptive optics compensates for atmospheric turbulence.
Sources & references elt.eso.org/about/ elt.eso.org/about/facts/ elt.eso.org/instrument/MICADO/
ASTRONOMY & SPACE
UPLIFT connects lightweight tank structures with cryogenic testing for liquid-hydrogen applications. CRYOVAC and ArianeGroup are development partners of DLR for the test rig.
Test before assembly DLR tests composite tank domes for structural performance and gas-tightness before assembly. Controlled cryogenic conditions help assess materials for future hydrogen aviation.
Sources & references event.dlr.de/ila2026/uplift-tank-test/ www.dlr.de/de/sy/forschung-transfer/forschungsinfrastruktur/projekt-uplift-saeule-c-kryogene-techniken
TEMPERATURE METROLOGY
Primary thermometry relates temperature to measurable physical quantities. Dielectric-constant gas thermometry uses the electrical response of a gas as pressure changes.
A stable experimental environment A cryostat provides controlled thermal conditions for the experiment. The papers explain measurement methods; their uncertainty figures do not specify this individual CRYOVAC system.
Publications Context & publication summaries 01 C. Gaiser, B. Fellmuth & N. Haft · 2008
Primary Dielectric-Constant Gas Thermometry in the Range from 2.4 K to 26 K at PTB A PTB study comparing primary gas-thermometry measurements with ITS-90 at low temperatures.
DOI 10.1007/s10765-007-0318-4 · International Journal of Thermophysics 29, 18–30
02 C. Gaiser, T. Zandt & B. Fellmuth · 2015
Dielectric-constant gas thermometry A review of the physical principles, experimental techniques and results of DCGT.
DOI 10.1088/0026-1394/52/5/S217 · Metrologia 52, S217–S226
Sources & references www.bipm.org/documents/20126/237262613/SI-App2-kelvin-2024-TG-Dig-revision/1444eda0-9ec1-7917-9eb7-41bc0d73e23a doi.org/10.1007/s10765-007-0318-4 link.springer.com/article/10.1007/s10765-007-0318-4 doi.org/10.1088/0026-1394/52/5/S217 www.ptb.de/cms/fileadmin/internet/publikationen/ptb_news/pdf/englisch/PTBnews_2016_1_e.pdf
TEMPERATURE METROLOGY
ITS-90 gives laboratories a practical temperature scale. PTB realises and transfers it using fixed points, gas and vapour-pressure thermometry, and resistance thermometers.
Scale and thermodynamic temperature Primary measurements allow comparison with thermodynamic temperature. Calibration then connects everyday thermometers to established reference measurements.
Sources & references www.ptb.de/cms/en/ptb/fachabteilungen/abt7/fb-74/ag-743.html
TEMPERATURE METROLOGY
Polarizability describes how a gas responds to an electric field. Knowing it accurately helps connect electrical measurements with pressure and temperature.
Helium, neon and argon The PTB study investigates these noble gases using dielectric-constant gas thermometry. The resulting reference data support gas metrology and tests of theoretical calculations.
Publications Context & publication summaries 01 C. Gaiser & B. Fellmuth · 2018
Polarizability of Helium, Neon, and Argon: New Perspectives for Gas Metrology Experimental noble-gas polarizability values for pressure and temperature metrology.
DOI 10.1103/PhysRevLett.120.123203 · Physical Review Letters 120, 123203
Sources & references doi.org/10.1103/PhysRevLett.120.123203 journals.aps.org/prl/abstract/10.1103/PhysRevLett.120.123203 tsapps.nist.gov/publication/get_pdf.cfm?pub_id=926683
Partner overview
Free-piston Stirling engines and cryocoolers.
CryoTel GT Stirling cooling in a compact package. The CryoTel GT from Sunpower delivers a nominal 16 W at 77 K with a reject temperature of 23 °C. We help define the configuration and integration for your application. The image shows the base model.
Nominal cooling capacity: 16 W at 77 K, reject temperature 23 °C Nominal input power: 240 W Power supply: 48 V DC Base model: 3.1 kg · 276 mm length · 83 mm diameter Partner overview
Superconducting magnets, cryogenic systems and related instrumentation.
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