Titlebook: Next Generation Infrared Space Observatory; S. J. Bell Burnell,J. K. Davies,R. S. Stobie Book 1992 Springer Science+Business Media Dordrec

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Optical Design and Testing of a Fast, Large Aperture, Infrared Space Telescope,um aperture 2.5 metre with an F/1.2 primary and wavelength coverage from λ = 2 to at least 40 .m, and possibly to 100 .m. Compactness, low thermal emission from the optics and structure, diffraction limited imaging at λ = 2 .m, and sensitivity to misalignment aberrations and manufacturing errors wer

Acetabulum

Closed Cycle Coolers for Space Applications,pment work is now concentrating on multistage coolers for temperatures below 30 K. This paper describes results from a two stage cooler built at the Rutherford Appleton Laboratory and preliminary tests on a closed cycle 4 K cooler.

patriot

Aspects of Data Flow for an Edison-Type Observatory,e in the near (2–50 .m) infrared and having a mission lifetime often to twenty years. This would be achieved using a passively cooled mirror and an instrumental package whose passive cooling is aided by a mechanical cooler. The data-flow to and from such a telescope would be large and thus the data-

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Factual

https://doi.org/10.1007/978-94-011-2680-9Evolution; astronomy; astrophysics; interstellar matter; observatory; star; star formation; telescope

Conduit

Infrared Space Studies of Solar-System Objects: The Post-ISO ERA,es. Beyond ISO, future Solar-System studies using infrared space missions will require an extension of the spectral coverage toward longer wavelengths and increased spatial capabilities for imaging spectroscopy.

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Stellar Infrared Astronomy with Edison,an be extracted from such observations. Some emphasis is placed on the possibilities of stellar IR astronomy using a large space-borne telescope, especially with respect to the much better spatial and spectral resolution of such a telescope compared to the current generation of ground-based and space IR telescopes.

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