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161. http://www.mso.anu.edu.au/~geoff/HEA/FRW.pdf
Cosmological Space -Times Lecture notes compiled by Geoff Bicknell based primarily on: Sean Carroll: An Introduction to General Relativity plus additional material Thursday , 10 September 2009 1 Metric of special relativity ds 2 = -c dt + dx + dy + dz 2 2 2 2 2 = -dx 02 + dx + dy + dz 2 2 2 = µ dx dx µ where µ µ, = = Minkowski tensor = diag [-1, 1, 1, 1] 0, 1, 2, 3 This is the metric of four-dimensional flat ... The 3-sphere is expanding 3. ...
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Ссылки http://www.mso.anu.edu.au/~geoff/HEA/FRW.pdf -- 1606.0 Кб -- 10.09.2009
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162. http://www.arcetri.astro.it/~olmi/GRASP/BLAST-01sep051.tor
BLAST_coor_plot coor_plot ( coor_names : sequence ( ref (BLAST_global_feed)) ) BLAST_freq frequency ( list_freq : sequence ( 580.2700000 GHz) ) BLAST_con_feed_250micron conical_feed ( aperture_radius : 1.200000000 mm, flare_length : 23.71040000 mm ) BLAST_global_feed coor_sys ( ) BLAST_source feed ( frequency : ref ( BLAST_freq ), coor_sys : ref (BLAST_global_feed), feed_definition : ...
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Ссылки http://www.arcetri.astro.it/~olmi/GRASP/BLAST-01sep051.tor -- 29.8 Кб -- 04.11.2005
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163. http://www.stsci.edu/science/preprints/prep1280/barnbaum.preprint.doc
... The primary channel receives the desired astronomical signal corrupted by RFI (radio frequency interference ) coming in the sidelobes of the main beam. ... If the interference-to-noise in the reference and primary channels are equal ([pic]), the noise in the system output (at the frequencies where the interference signal was located) will be almost twice as high as in the primary input before filtering. ... The signal path through the adaptive filter illustrates the iterative nature of this system. ...
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Ссылки http://www.stsci.edu/science/preprints/prep1280/barnbaum.preprint.doc -- 312.0 Кб -- 01.09.1998
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164. Sloan Digital Sky Survey 2.5-meter telescope: optics
Sloan Digital Sky Survey Telescope Technical Note 19980416 . ... The common corrector . ... The Sloan Digital Sky Survey (SDSS) 2.5-meter telescope optical design is optimized for wide field (3њ), broadband (300 nm to 1060 nm) CCD imaging and multi-fiber spectroscopy. ... The second corrector element figure is in the negative of the usual form and placed closer to the focal plane. ... Grind and figure flat silica corrector for the Sloan Digital Sky Survey Telescope - Corrector Final Report", (1997). ...
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Ссылки http://www.apo.nmsu.edu/Telescopes/SDSS/eng.papers/19980416_Optics/19980416.html -- 42.5 Кб -- 08.09.1998
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165. http://www.mrao.cam.ac.uk/~anthony/anl.pdf
Conformal Geometry and the Universe B y Anthony Lasenby Astrophysics Group, Cavendish Laboratory, Madingley Road, Cambridge CB3 0HE, UK The conformal approach to Euclidean geometry introduced by David Hestenes, uses null vectors in an enlarged space to represent points. ... The conformal model for the geometry of Euclidean space was introduced by David Hestenes (Hestenes 2001), and has been discussed further by several authors (see e.g. Lasenby & Lasenby 2000 and Hestenes et al. ...
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Ссылки http://www.mrao.cam.ac.uk/~anthony/anl.pdf -- 379.8 Кб -- 28.08.2004
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166. http://star.arm.ac.uk/preprints/400.pdf
... Soc. 339, 524н536 (2003) Anatomy of the HerbigнHaro object HH7 bow shock Michael D. Smith, 1 2 1 Tigran Khanzadyan 1 and Christopher J. Davis2 Armagh Observatory, Armagh, Northern Ireland, BT61 9DG пп Joint Astronomy Centre, 660 N. A'ohoku Place, University Park, Hilo, Hawaii 96720, USA Accepted 2002 October 18. ... We first present molecular hydrogen images in the 2н1 S(1) and 1н0 S(1) K -band emission lines. ... 3 OBSER VA TION AL RESUL TS Fig. 1 displays the HH7 bow shock in detail. ...
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Ссылки http://star.arm.ac.uk/preprints/400.pdf -- 984.7 Кб -- 17.09.2003
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