Download Into Battle!: British Orders of Battle for the Crimean War, by Ron McGuigan PDF

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Extra resources for Into Battle!: British Orders of Battle for the Crimean War, 1854-56

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These features appear between the absorption produced by CH 4 and that of the poly-acetylenes. The region above 8 /-lm (see Figure 5b) presents some weak bands that certainly arise from heavy species. 5. Mid-Infrared spectrum of CRL618 at selected wavelengths. The thin line in each panel corresponds to the model of Cernicharo et al. (2000b). 27 /Lm corresponds to the symmetric bending of CH3. The broad range of absorption bands produced by wagging and twisting of CH2 in small hydrocarbons is indicated by the horizontal line (from Cernicharo et al.

2 TELESCOPE The SOFIA telescope is a Cassegrain system with Nasmyth focus (see Fig. 4). 7 m. 5 m. The mirror is made from Zerodur (Schott). This material has an extremely low thermal expansion and provides sufficient stiffness for use in an aircraft environment. A honeycomb structure is milled into the rear side of the mirror. This makes it the largest lightweighted mirror in the world. 3 Jlm. The hyperbolic secondary mirror (M2) has a diameter of 35 cm. It is made from silicon carbide. The secondary mirror is attached to a chopping mechanism which provides chop amplitudes up to ±5 arcmin at chop frequencies up to 20 Hz.

A similar mission, the Swedish-French ODIN satellite will be launched soon (2002). Both missions carry telescopes with a diameter of about I m and are equipped with heterodyne receivers which are optimized for the observation of 45 molecular oxygen and water in galactic sources. ODIN will also be used for the investigation of Earth's atmosphere [2]. Within the next ten years four major satellite missions are in preparation. The Submillimeter and InfraRed Telescope Facility (SIRTF) will be launched in 2002.

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