... Up: Science Data Pipelines . ... The Chandra Automatic Data Processing System (AP) requires quick access to previously generated data. ... This archive interface layer includes an archive request queue, a data archiving server (darch), and an archive ``cache''. ... In our implementation, the cache is actually a directory where the data files reside, as shown in Figure 1 . ... If the data products are not in the cache, then the pipeline retrieves the files from the archive database. ...

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Static Fourier spectrometers are often used for spectral measurements of the ionosphere emissions. There are two main advantages of Fourier spectrometers (FS) - large geometric factor and high spectral resolution; these parameters are two orders better than for grating spectral instruments. ... In scanning Fourier spectrometer optical and electric modulation of signal is used to avoid this problem, for static Fourier spectrometer there are no such ways. ...

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So how do we find objects on the other side of the Universe? ... The latest instruments enable us to scan large areas of sky. Using Cerro Tololo's Blanco 4m telescope and the Canada-France-Hawaii 3.5 metre telescope , we are able to scan a piece of sky larger than the size of the moon every 5 minutes to a faintness level which allows us to find Type Ia supernovae halfway across the Universe. Type Ia supernovae are very rare - but each image we take contains 50000 galaxies. ...

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... TD = Minimum cost for a possible transformation of s into t. Any transformation which gives this minimum is called an optimal transformation. ... The running time is given by: O((m'3+n'3)|Alpha|+mn'2+nm'3+mn) A different look at Duplication History s 1 s2 s 3 s 4 s 5 s 6 s 7 s 8 s 1 s 2 s 3 s 4 s5 s 6 s 7 s 8 observed s s Right duplication Left duplication Right duplication Left duplication Right duplication Right duplication Right ...

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Beginning from the May of the 1997 we started to publish our daily solar radio observations at RATAN-600 radiotelescope. ... Periscope System: South Sector+Flat Mirror . ... It is possible to track a source by moving the secondary mirror along the arc-shaped railway tracks or to perform azimuthal 2D map synthesis . ... 1) It is possible to simultaneously carry out independent observing programs using individual sectors at various discrete azimuths and secondary mirrors on corresponding railway tracks. ...

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DIGITELTM ION PUMP CONTROLLERS DIGITELTM ION PUMP CONTROLLERS DIGITELTM ION PUMP CONTROLLERS The DIGITEL family of Ion Pump controllers of fers the right balance of per formance, power and protection. DIGITELTM SPCe | Small Pump Controller The SPCe is a versatile way to fully operate ion pumps 0.2 ­ 75 l/s. An LCD pressure/current/voltage display along with standard serial communications makes the SPCe able to accommodate the needs of basic and advanced users. ... DIGITELTM MPCe | ...

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To main of Laboratory . The research work and design of optical and optical-electronic devices are carries out by laboratory staff: . ... Lens: . ... In the layout 1 prism systems perform functions of dispersive element, corrector of aberrations, optical reducer. ... Spectral range 200 - 400 nm; . ... Back Forward . ... The main corrector's function are compensation of field aberrations of the main spherical mirror of a telescope (diameter of 600 mm, f'=1200 mm) and increase aperture ratio. ...

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