Next: File Formats Required Up: OPTOPUS Commands and Previous: Optopus commands . Below follows a description of all parameters that can be set by the SET/OPTOPUS command, the commands which use these parameters and the default values. ... If an OPTOPUS command the default value is not used the command will, in addition to actual OPTOPUS operation, also overwrite the setting of this parameter and hence will change the default value. ... set the equinox . ... Table: Command parameters . ...

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• ANALYSE/ROMAFOT
• Order definition: Method Hough
• Starting up

... CentralProcessor 0.11 documentation . ... The Central Processor Manager is the local monitoring and control agent for the Central Processor sub-system. ... At the moment the Central Processor Manager only controls the acquisition phase; that is, it only controls the ingest pipeline. ... In addition to the CP manager specific parameters, any parameters that begin with ice_properties are passed directly to the ICE Communicator during initialisation. ... string . ... Central Processor Manager . ...

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• cmodel (Model Image Generator) CentralProcessor 0.11 documentation
• ccontsubtract CentralProcessor 0.11 documentation
• User Parameters - Mosaicking Continuum images CentralProcessor 0.11

... Chapter 10: Fine Guidance Sensors (FGS) > 10.2 Mode = POSConfig = FGS . ... 10.2.5 Time Per Exposure . ... In addition, a few stars (reference and/or target) should be observed multiple times during a visit to map any positional drift of the field due to HST pointing characteristics (see the FGS Instrument Handbook) . ... The default values of the Optional Parameters are set in this Mode to provide acceptable data for single, zero angular diameter stars. ... NULL . ... The default value is 15 arcsec...

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• Obsolescent Acquisition Parameters
• Mode = TRANSConfig = FGS
• Index

... Meta Index / Home Page / Usage / Command-line lists of parameters . Whilst there are a large number of command-line parameters, frequently many of them will not be required. ... The parameters imageset , oldsrclistset and newsrclistset are always required. The parameters sourceno and phototype are always required. ... If more than one source is listed in the parameter sourceno then the length of the lists of each photometry parameter must be the same as the number of the sources. ...

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• OPERATION
• Source shape parameters (semi-major/minor axes and position angle)
• Procedure

... rotang, Date, RA, Dec, Time, accS, ast=ast, ha=ha, lst=lst, jd=jd, az=az, za=za, sep=sep, rotang=rotang, alfabeams=alfabeams . ... It is thus possible to specify, for instance: rotang, ... , ha=haHr, lst=lstHr, ast=astHr . ... alfa_angle - script to launch the GUI . alfa_ang.pro - the GUI: provides input to rotang and a graphical display of the results. rotang.pro - the main routine of the program: finds the required time, the other associated times, Az and ZA using ao_idl routines. ...

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• Rotang - IDL procedure for calculating the optimum rotation angle for ALFA
• AGES Database Search
• Converting Arecibo Interim Correlator data into a FITS image

Instructions for using Menu-driven Axis Control Software . ... Altitude and azimuth axes use position feedback and the setting is in counts per second times 10. ... Use b to set the brakes and use c to clear the brakes for the corresponding axis, either azimuth or altitude. ... Use m to move to the previously specified position and velocity for the corresponding axis; either azimuth or altitude. ... Use g to move to the previously specified position and velocity for both the azimuth and altitude axis. ...

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• Untitled Document
• Procedure to Install the 2.5m Secondary Truss
• Procedure to Collimate the SDSS 2.5m Secondary Mirror

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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• Working with
• HSTPOLSIM (V2.00) --- November00 --- HSTPOLSIM (V2.00)
• Plot data from the WDS

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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• HSTPOLSIM (V1.00) --- April99 --- HSTPOLSIM (V1.00)
• stecf.impol - Package Tasks
• HSTPOLPOINTS (V1.00) --- May99 --- HSTPOLPOINTS (V1.00)

Region markers can be moved, resized, rotated, zoomed, deleted, and can change geometric type. ... For example, markers placed on astronomical catalog positions should be fixed so that one cannot accidentally move them off the specified position. ... Parameters can be fixed using the fix option of the regions public access point (for fixing classes of markers) or by means of a fix keyword in the definition of an externally loaded marker. ... In the command: echo "regions fix all -position -size" | ...

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• QPOE Files
• Summary of Tasks in This Section
• Possible Pitfalls

Stellarium 0.12.3 . ... Classes . ... ClassљList . ... Refraction Class Reference . ... virtual voidљ . forward ( Vec3d &altAzPos) const . ... backward ( Vec3d &altAzPos) const . Remove refraction from position ("reduce"). ... forward ( Vec3f &altAzPos) const . ... setupGLSLTransform ( StelGLSLShader *shader) . ... virtual void Refraction::backward . ... virtual void Refraction::disableGLSLTransform . ... virtual void Refraction::forward . ... virtual void Refraction::setGLSLUniforms . ...

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• Stellarium: TextParams Struct Reference
• Stellarium: SphereParams Struct Reference
• Stellarium: RingParams Struct Reference

... The HST uses an onboard model of its orbit to perform in real-time various control functions relating to spacecraft operations and observation support. ... New coefficients for the ephemeris are updated every other day, and are archived as FITS keywords for each HST observation data set. Using these coefficients,an observer can perform a variety of calibration and characterization calculations relating to the orbital position and velocity of the telescope. ...

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• Multiwave Continuum Data Reduction at RATAN-600
• Enhanced HST Pointing and Calibration Accuracy: Generating HST Jitter Files at
• TwoFitlines: An Spectrum and Line Analysis Tool

... JavaScript 1.1: added current, next, and previous properties. ... To change a window's current URL without generating a history entry, you can use the Location.replace method. ... For example, if the history list contains three named entries, these entries are reflected as history[0] , history[1] , and history[2] . ... back . ... onClick="history.go('home.netscape.com')"> The following button navigates to the URL that is three entries backward in the history list: <P><INPUT TYPE="button" VALUE="Go" ...

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• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/fileup.htm
• Program parameters
• mod_session_crypto - Apache HTTP Server

... The package AMPLE (Adaptable Minor Planet Ephemerides) is dedicated to solving a number of problems concerning minor planets with the aid of IBM-type personal computer. ... Obtaining selection of orbital elements and/ or photometric parameters of minor planets in conformity with imposed restrictions. ... The orbital elements of all minor planets used in AMPLE for 2015 have been determined in IAA on the ground of available observations in the catalogue of observations of the Minor Planet Center. ...

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• ENGAMPLE
• NAA-2

... The predicted MIR's ground tracks, which pass near INSPIRE net, are available in this home page. The track consists from magnetic footprints calculated by magnetic mapping from MIR positions with 30 s step. ... For each time some of the INSPIRE net place are selected as soon as its coordinates are close to the MIR magnetic footprint (the geocentric angular distance between SP and footprint is less then 2.1 deg) . Back to the Top . ... Back to the IKI Satellite Situation Center (SSC) . ...

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• Satellite position in the SE and GSM coordinate systems
• STDA files
• Magnetic mapping

... spectrum . ... sfit . ... Briefly, these refer to the type of spectrum to be computed, the method of calculation of the source function, the number of anges if specific intensities are to be computed, the choice of continuous opacity subroutine library, the broadening data for HeI lines and the approximation ito be used for untabulated diffuse HeI lines. ... Refer to the SPECTRUM documentation for more information. spc_nsource <nsource> : Switch for method used to compute source function (def: 3) . ...

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• SCL Sfit SLV Commands
• Sfit Control Language: Classified Listing
• sfit help file

Fortran 90 properties already in CF77 . ... Only the old form (fix form) of the source code is available. ... LOGICAL Default KIND number = 8 INTEGER Default int7 int15 KIND number = 6 1 2 digits = 46 7 15 radix = 2 2 2 range = 13 2 4 huge = 70368744177663 127 32767 bit_size = 46 8 16 INTEGER int31 int46 int64 KIND number = 4 6 8 digits = 31 46 63 radix = 2 2 2 range = 9 13 18 huge = 2147483647 70368744177663 9223372036854775807 bit_size = 32 46 46 REAL half Default,single double KIND ...

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• Keyword arguments and default arguments
• Notation
• Tutorial on Fortran 90, Digital UNIX

... Calculations of at least two runs with different values of a parameter are required in order to discover to what extent the results depend on the , if at all. ... In order to study how the final statistical distributions depend on the initial functions, the method of Green functions is used. ... Then we can restore any distribution on this parameter (with a certain accuracy) by summing the results for each interval with the appropriate weight. ...

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• Initial Distributions of Binary Parameters
• Initial parameters of compact stars
• Notes on Monte-Carlo Simulations

OFFICIAL PRESS RELEASE . ... the International Space Station . ... P. Semenov, Technical Manager of the Russian Manned Space Programs, General Designer of S.P. Korolev RSC Energia, Academician of the Russian Academy of Sciences, Frederick D. Gregory, NASA Deputy Administrator, N.A. Anfimov, General Director of TsNII of Machine-Building, Academician of RAS, as well as representatives of Roskosmos, NASA, Russian enterprises and organizations participating in the implementation of the ISS program. ...

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• INTERNATIONAL SPACE STATION
• VIDEOARCHIVE. THE SECOND PRIME MISSION TO THE INTERNATIONAL SPACE STATION
• S.P.Korolev RSC Energia - ECOLOGICAL MONITORING

... Impact of Covariance Information on the Orientation Parameters Between Radio Source Position Catalogs, IVS 2012 General Meeting Proceedings, p.339­341 http://ivscc.gsfc.nasa.gov/publications/gm2012/sokolova.pdf Impact of Covariance Information on the Orientation Parameters Between Radio Source ... IVS Analysis Centers provide these catalogs in a standard IERS format, where together with radio source positions and other relevant information, RA/DE correlations are reported. ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf
• Pulkovo NEO Page: Ephemeris Support

... This appartus will drop a mass from different heights. When the mass strikes the ground, some percentage of its original energy will be absorbed by the ground. ... The percentage of the energy which is absorbed by the surface on each "bounce" (EAS) . ... The impact velocity of the object will also be given at each bounce. ... Start= Drop the ball after Energy, Mass and EAS have been set; resume after step or pause has been selected . ... Reset = Reset experiment to intial values . ...

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