The following parameters as a function of the universal time are enclosed in this file. 1. no . ... Universal time date (YYYYMMDD) . ... Universal time (.hhmmss) . ... Geomagnetic local time in the satellite position . ... geomagnetic latitude . ... co-ordinate - . ... system . ... co-ordinate system . ... Solar-ecliptic co-ordinate - . ... Satellite velocity . ...

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• Satellites commerciaux

... News Latest News News Archive Newsletter Quarterly Status Report . ... Data Analysis SAS News What is SAS? ... Archive, Pipeline & Catalogues XMM-Newton Science Archive Pipeline Processing System Observation Data Status Time Correlation Fix Serendipitous Source Catalogue OM Serendipitous Source Catalogue Slew Survey Catalogue Latest Slew Results Browsing Interface for RGS Data Live Radiation Monitor Plots Radiation Monitor Files . ... Please refresh your browser to update the satellite position. ...

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• srcinfov: compute position of SouRCe in Field Of View

Program: TRACE Purpose: TRACE plots image values at user given positions as function of distance to a plot centre (in 2-d (sub)sets). Category: ANALYSIS, PLOTTING File: trace.c Author: M.G.R. Vogelaar Keywords: INSET= Give set (, subset): Only one subset is allowed. ... XYBOX= Give size of box around one pixel: [3,3] The resulting value at a selected position is an average of the pixels in the defined box around that position. ... POSITION= Give position x, y: Physical values are allowed. ...

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• Satellite Tracking
• WCSLIB: sph.h File Reference
• kpvslice: interactive position-velocity slicing

Natural Satellites Service. ... Apparent Encounters . of the Tycho-2 Catalogue stars and the main natural planetary satellites . ... Suggestions . ... Here we present the precalculated circumstances of the apparent encounters of the stars of the Tycho-2 Catalogue with the main satellites of Saturn (S1-S8) for the period from November 2004 to February 2010, and with the Galilean satellites of Jupiter for the period from November 2004 to October 2010. ...

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• IMCCE-SAI: Natural Satellites Service. Ephemerides. Satellites lointains de
• IMCCE-SAI: Natural Satellites Service. Ephemerides. Satellites de Saturne
• IMCCE-SAI: Natural Satellites Service. Ephemerides. Satellites de Pluton

... With enough velocity, a spacecraft can break loose from the Earth's gravity and enter an orbit around the Sun, like that of a planet. If it then orbits the Sun with the same period as the Earth--one year--it may keep a fixed position relative to Earth. ... If the distance is just right--about 4 times the distance to the Moon or 1/100 the distance to the Sun--the spacecraft, too, will need just one year to go around the Sun, and will keep its position between the Sun and the Earth. ...

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• Satellites with commercial missions
• Corrected Geomagnetic Coordinates
• The Favourable Spatial Position Criteria

. Next: Initial velocity Up: Space and velocity distributions Previous: Space and velocity distributions . Following Paczynsky (1990), we assume initial space distribution of young neutron stars to be varying exponentially with distance from the Galactic center and from the Galactic plane, that is probability distribution for young neutron star positions can be written in the form . with kpc, and pc. Mike E. Prokhorov . Fri Jul 19 19:16:07 MSD 1996

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... Positions in 2000 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2001 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2002 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2003 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2004 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . ...

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• PhD position, Centre for Astronomy, NUI Galway: deadline 18 July 2008 |
• Postgraduate Positions
• The Human Orrery

... The amount of energy encircled by an aperture used for stellar photometry will depend on both the aperture size, and also on any variations in the PSF with field position, time, etc. ... The differences in photometric magnitude between apertures with various radii (i.e. aperture corrections), and their mean and standard deviations for the F555W filter, are presented in Table 5.5 . ... Variations in the PSF with field position will, of course, cause a position dependence in the aperture corrections. ...

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• Chapter 4: Solar System Targets
• CCD Position and Orientation on Sky
• PMSU2 - Table 1B

On,off position switching is done to remove standing waves from the resulting spectra. ... 1,5,10,20,25,50,100 samples corresponding to great circle angular offsets of .004,.02,.04,.07,.09,.18, and .35 degrees. ... Page 1: rms vs great circle offset. ... Page 2: rms vs little circle offset. ... The rms increase correlates better with great rather than little circle offsets. the 1 usec standing wave starts to be seen in the .07 degree offsets. a .9 usec standing wave is seen at .35 degrees offset. ...

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• glonass satellites
• sband_moon_test
• Test of Position Switching with a Specified Off Position

. Computer Ephemeris. Lunar equatorial positions. Explanations. Each row contains at 0 h and 12 h of Time Dynamical Terrestrial: month, day, apparent right ascension (hours, minutes, seconds), apparent declination (degrees, minutes, seconds of arc) and geocentric distance (in Earth's radii).

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• Central meridian positions for physical observations of Saturn for Computer
• Central meridian positions for physical observations of Uranus for Computer
• Central meridian positions for physical observations of Neptune for Computer

Swift Launches . ... Credit Copyright: NASA Explanation: Where do gamma ray bursts occur? To help find out, NASA launched the Swift satellite on Saturday, as pictured above . What Swift is designed to do better than any previous satellite is to quickly locate these enigmatic explosions in both sky position and distance. Once a gamma ray burst (GRB) is located, Swift itself will rotate to face it head-on and determine its distance directly. ... NASA Official: Jay Norris. ...

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• Swift Launches
• Optical Transient Near GRB970508 Shows Distant Redshift
• XWare > APOD

... 8, ``Celestial Mechanics'', 2002 CCD observations of planetary satellites and occultations and close approachments of stars by asteroids with 26­ inch refractor of Pulkovo observatory T. P. Kiseleva, I. S. Izmailov, M. A. Mozhaev Pulkovo Observatory, St. Petersburg, Russia ST--6 CCD camera has been used with 26-- inch Refractor at Pulkovo for ob­ servations of ... These estimates are \Sigma0:015 arcsec and \Sigma0:014 arcsec for X and Y correspondingly. ...

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• http://www.ipa.nw.ru/conference/2002/sovet/PS/KESHIN.PS
• LAB Ephem. Astronomy-ERA
• AY2016 (contents)

Prognoz-6 satellite position data . Filename from to size . F770922.POS 22-09-77 03:00 30-09-77 22:00 13.7k . F771001.POS 01-10-77 00:00 31-10-77 22:00 47.7k . F771101.POS 01-11-77 00:00 30-11-77 22:00 46.1k . F771201.POS 01-12-77 00:00 31-12-77 22:00 47.7k . F780101.POS 01-01-78 00:00 31-01-78 23:00 47.7k

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• Empirical Model of the Nighttime Winter Ionospheric Trough

... 2004 November 22 . Swift Launches . Credit: NASA . ... To help find out, NASA launched the Swift satellite on Saturday, as pictured above . ... Once a gamma ray burst (GRB) is located, Swift itself will rotate to face it head-on and determine its distance directly. ... Subsequently collected GRB and afterglow information will help astronomers not only determine the nature of the initial explosions, but also the nature of the expanding shockwaves. ... About APOD | ... NASA Official: Jay Norris. ...

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• APOD: May 13, 1997 - Optical Transient Near GRB970508 Shows Distant Redshift
• Further Information and Bibliography

- the current position of the "Universitetskiy" satellite'> . Your browser does not support inline frames :( It must be a very old one. Upgrade to Microsoft Inrernet Expolorer 4 or later, Netscape 6 or later etc. Skobeltsyn Institute of Nuclear Physics.

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• University Satellites and Space Science Education '2006
• UNIVERSAT-2009: University Satellites in Space Sciences Education, Zvenigorod,

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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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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• ESO - ALMA
• The ArTeMiS cryostat in position at APEX
• Position of the quasar 3C 279 in the constellation of Virgo

Next: Catalog Construction Up: Observations and Analysis Previous: Source Detections . ... It was assumed that the highest signal gives the most likely position of the source. ... Comparing the summed map with the maps from the individual energy ranges, the one which produced the smallest error box was chosen to represent the source position, as long as was greater than 4, a level chosen to reflect a reasonable degree of confidence in the detection. ...

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• Arcsecond Positions of UGC Galaxies
• HyperLEDA documentation: compilation of distance measurements (a007)
• Dome position.

This composite shows the alignment of the satellite galaxies of Andromeda in relation to the view that we see from Earth (the top left panel shows a true-color image of the center of the Andromeda Galaxy taken with the CFH Telescope). New distance measurements allow us to ascertain the 3-D positions of the satellite galaxies, which together with new velocity measurements, reveal their true nature as part of a gigantic rotating structure (side view: bottom left panel; front view: top right panel). ...

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B057758EC-8CE7-457F-A58D-7B6DEF643344%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B47B9C495-380F-4DB6-A758-353B159D94BE%7D
• Mars orbiter repositioned to phone home Mars landing | Astronomy.com

Stellarium 0.12.3 . ... Classes . ... gSatTEME Class Reference . Sat position and velocity predictions over TEME reference system. ... Set compute epoch for prediction. ... gVector љ . ... Get the TEME satellite position Vector. ... Get the Geographic satellite subpoint Vector calculated by the method compute SubPoint. ... gVector Satellite position vector meassured in Km. x: position[0] y: position[1] z: position[2] . ... gVector Satellite Velocity Vector measured in Km/s x: Vel[0] . ...

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• Stellarium: Skybright Class Reference
• Stellarium: Nebula Class Reference
• Stellarium: Position Struct Reference