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• http://www.atlasaerospace.net/eng/online-ssop.htm
• http://www.atlasaerospace.net/eng/sitemap.htm
• Plan and technical specifications of the Baikonur cosmodrome, Russia's space

This diagram illustrates the effects of absolutely positioning a box ("inner") with respect to a containing block established by a relatively positioned ancestor ("outer"). ... The "inner" box has been positioned relative to the top and left edges of the "outer" element's first inline box. ... The reference edges for positioning the "inner" box are indicated in the diagram by thick dashed lines. ... 1 Beginning of body contents.| ... 4 [(+200, -100)] 5 Inner 6 contents. ... Inner contents" is blue. ...

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• Long description for example illustrating absolute positioning
• Long description illustrating absolute positioning with respect to the initial
• Long description for relative flow example

Table 4.1: Solar System Standard Targets . Table 4.2: Target Description Keywords . Table 4.3: Positional Parameters for TYPE = COMET . ... Observers for solar system Targets of Opportunity (e.g. a "new" comet or asteroid, a solar-wind disturbance reaching the Jovian magnetosphere, etc.), should complete the Generic Target List ( See 3.12 Generic Targets List [Generic_Targets] ) and the Visit and Exposure Specifications (to the extent possible) in time for the Phase II deadline. ...

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• Chapter 3: Fixed and Generic Targets
• Chapter 3: Fixed and Generic Targets
• Fixed and Generic Targets

... Given an image covering some part of the sky, and a list of sky positions, it can be useful to know the value of the image at each of the positions in the list. The image might be a sensitivity or an exposure map for example: one might want to translate this into sensitivity or exposure at each of the positions. ... At present, the list of positions (which must be a binary table extension in a FITS file) must contain columns which give the position in image pixel coordinates. ...

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I/146 Positions and Proper Motions (Roeser+ 1988) ================================================================================ Catalogue of Positions and Proper Motions Roeser S., Bastian U. =1988A .. ... 449R ================================================================================ ADC_Keywords: Positional data; Proper motions Description: PPM North gives J2000 positions and proper motions of 181,731 stars north of -2.5 degrees declination. ... The mean epoch is near 1931. ...

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• Positions and Proper Motions - South
• Supplement to the PPM Star Catalogue

Stellarium 0.12.3 . ... Classes . ... FileљStructure . ClassљList . ClassљIndex . ClassљHierarchy . ClassљMembers . List of all members | ... Position Struct Reference . ... More... #include < InterpolatedPosition.hpp > . ... Definition at line 37 of file InterpolatedPosition.hpp . The documentation for this struct was generated from the following file: . home/aw/devel/stellarium/trunk/plugins/TelescopeControl/src/clients/ InterpolatedPosition.hpp . ...

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• Stellarium: InterpolatedPosition Class Reference
• Stellarium: VertexP3T2 Struct Reference
• Stellarium: VertexP3T2C4 Struct Reference

... Co-ordinate systems description . Directories structure . The file names' construction . The file set description . ... The orbital information for each month is presented in the separate directory. The INTERBALL orbital data are located on the STDA server, for each month in the separate subdirectory, which name consists from the year (YYYY) and month (MM) numbers. The Parent Directory of the Tail Probe orbital data is http://www.iki.rssi.ru/da/interball/tail/orbit/ . ...

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• The FSP ASCII file description
• STDA files
• The numerical file description

... 330Wright+ J/MNRAS/251/330 8400MHz flux densities for Southern sources (Wright+ 1991) ============================================================================= Flux densities at 8400MHz for a large sample of radio sources WRIGHT A.E., WARK R.M., TROUP E., OTRUPCEK R., JENNINGS D., HUNT A., COOKE D.J. =1991MNRAS.251.. 330W ============================================================================= Description (Summary): We present 8400-MHz flux densities for 1194 southern radio sources. ...

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• General Description
• A VLA Survey of the First Quadrant of the Galactic Plane at 1.5
• Arcsecond Positions of UGC Galaxies

Ground Support of RadioAstron . Control and Tracking Stations . RadioAstron satellite control (command transmission, telemetry, orbit measurements) will be conducted from Evpatoria and Bear Lake control stations. ... Coarse orbit measurements will be carried out from control stations. Each measurement takes ten minutes. ... Orbit measurements at tracking stations give only radial component of spacecraft velocity but the measurements are going continuously during observing sessions. ...

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• Description of the RadioAstron project, russion version

... Description . Catalog . ... In the Catalog, we publish equatorial (ЮБ 2000 , ЮД 2000 ) and galactic (l,b) coordinates of cluster centers derived as the position of overdensity in 2MASS catalog (Koposov et al. ... Distances, color-excesses and ages are the mean-square values calculated using all available evaluations from different color-magnitude diagrams. ... There are individual pages for every cluster where all available plots and parameters are published. ... 2002). ...

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Name: PGBAND Purpose: read cursor position, with anchor Category: GRAPHICS File: pgplot.src Author: T.J. Pearson Use: see description below. Description: INTEGER FUNCTION PGBAND (MODE, POSN, XREF, YREF, X, Y, CH) INTEGER MODE, POSN REAL XREF, YREF, X, Y CHARACTER*(*) CH Read the cursor position and a character typed by the user. ... If MODE=3, two horizontal lines are extended across the width of the display, one drawn through the anchor point and the other through the moving cursor position. ...

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• http://www.atnf.csiro.au/computing/software/gipsy/sub/pgcurs.dc2
• The Local Volume HI Survey (LVHIS)
• casacore: casa::RegexBase Class Reference

Multichannel Flare Spectrograph . ... phi - the angle between the green vertical line passing through the solar disk image and the violet radius vector "r" of the object located at the center of the spectrograph slit- red cross. positive - clockwise, negative - counterclockwise . ... mx = x coordinate of the coelostat main mirror . ... x : carthesian solar coordinate alog axis parallel to solar equator (in arcsec) . y : carthesian solar coordinate alog axis parallel to solar axis (in arcsec) ...

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fitcircle - find mean position and pole of best-fit great [or small] circle to points on a sphere. fitcircle [ xyfile ] -L norm [ -H [ nrec ] ] [ -S ] [ -V ] [ -: ] [ -bi [ s ][ n ] ] fitcircle reads lon,lat [or lat,lon] values from the first two columns on standard input [or xyfile ]. ... Then two locations are found: the mean of the input positions, and the pole to the great circle which best fits the input positions. ... If no file is specified, fitcircle will read from standard input. ...

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• http://xray.sai.msu.ru/~ivan/gmt/man/grdtrack.html
• http://xray.sai.msu.ru/~ivan/gmt/man/blockmode.html
• http://xray.sai.msu.ru/~ivan/gmt/man/blockmean.html

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

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• POLIMPLOT (V2.00) --- November00 --- POLIMPLOT (V2.00)
• HSTPOLSIM (V2.00) --- November00 --- HSTPOLSIM (V2.00)

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

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• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)
• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)
• POLIMPLOT (V1.00) --- April99 --- POLIMPLOT (V1.00)

... Karpachev A.T., IZMIRAN, e-mail: karp@izmiran.ru . ... The empirical median model of the shape and position of the MIT (Main Ionospheric Trough) in the Northern and Southern Hemispheres is presented. ... Geomagnetism and aeronomy, v.26, ? ... Karpachev A.T., Afonin V.V. Dependence of the ionospheric trough occurrence probability on the season, local time, longitude, and level of magnetic activity Geomagnetism and aeronomy, v.38, ? ... Karpachev A.T. Characteristics of a Ring Ionospheric Trough. ...

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• Ionosonde PARUS. Instrument Description.

RTT150 . ... The primary mirror 1 reflects light to the secondary mirror 2 which sends the converging beam of light to the system of four flat mirrors 3, 4, 5 and 6. That allows the beam of light to leave the telescope strictly along its polar axis and be collected in Coude focus. ... That's why at any tube position (for any rotation along the declination axis) beam of light parallel to the principal axis after reflection on mirror 3 follows the direction of declination axis. ...

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... Description . ... The SCORPIO-2 project: . ... The multi-mode spectrograph SCORPIO-2 was developed using the experience of observations at the 6-m telescope BTA with the SCORPIO focal reducer . ... The focal reducer consists of several units ('floors') mounted in the common case in the following order (from the telescope focal plane): . ... The focal reducer is connected with the platform-adapter which used for guiding by offset stars and for illumination the spectrograph by calibration lamps. ...

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• Format of data description
• V.Shergin's Home Page

The following papers summarize the characterization and technical performance of IBIS : . ... Characterization of Fabry-Perot interferometers and multi-etalon transmission profiles. ... Righini, A., Cavallini, F., Reardon, K. P., 2010, Astronomy and Astrophysics , 515 , A85, . ... The filter wheel is located between the two interferometers. ... The interferometers can be rapidly tuned, simultaneously, so to allow sequential scanning of the spectral lines of interest (see movie in IBIS Intro ). ...

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• Program parameters
• Luna 20
• Algorithm

... In the above example, the second region uses the global coordinate system (PHYSICAL by default). ... Supported systems include: name description ---- ----------- PHYSICAL pixel coords of original file using LTM/LTV IMAGE pixel coords of current file FK4, B1950 sky coordinate systems FK5, J2000 sky coordinate systems GALACTIC sky coordinate systems ECLIPTIC sky coordinate systems ICRS currently same as J2000 LINEAR linear wcs as defined in file In addition, two mosaic coordinate ...

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• Spatial Region Boundaries
• Journal of Young Investigators ( JYI )
• The SAOimage Menu (options within SAOimage)