A review of the NASA/OAST cryogenic coolers technology program

Physics

Scientific paper

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Coolers, Cryogenic Equipment, Heat Exchangers, Joule-Thomson Effect, Nasa Programs, Radiant Cooling, Adiabatic Conditions, Carnot Cycle, Demagnetization, Liquid Helium, Solidified Gases, Supercritical Pressures, Superfluidity

Scientific paper

Low and ultra low temperature cryogenic cooler systems for future space missions include mechanical, solid cryogen, gas adsorption, superfluid helium, helium-3, and magnetic (adiabatic demagnetization) coolers. Operating lifetimes required vary from a few weeks for a Shuttle/Spacelab mission to as long as nine years for missions to the outer planets. Temperature requirements vary from tens to tenths of kelvin. At the higher temperature, cooling loads for detectors, instruments and associated shields may be as high as 15 watts. The general requirements for low and ultra low temperature and techniques that can be employed to achieve these temperatures at expected heat loads are discussed. The NASA Centers involved in the R & T efforts and the type of cooler systems on which they are focusing their effort are considered as well as the thrust of R & T effort for each cooler type. Projected missions that will use the technology are identified.

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