... Source definition list: a dataset containing the SRCLIST table, and to which the region extensions will be added. evlist . ... The dispersion-axis spacing of vertices for image regions and the spatial background region, specified as the number of vertices across a node. ... Downward size of image regions, specified by the percentage of the cross-dispersion PSF covered between the source cross-dispersion off-axis angle and the lower of each pair of vertices with the same dispersion coordinate. ...

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• Description

... ACQ-DIST Optional Parameter for FGS 1 , 2 . ACQTYPE Optional Parameter for STIS . Acquisition modes . ... Aperture Coordinate System . ... AFTER date Special Requirement . ... BINAXIS1, BINAXIS2 Optional Parameters for STIS 1 , 2 . ... BUFFER-TIME Optional Parameter for STIS . ... CHECKBOX Optional Parameter for STIS . ... Calibration Targets . ... CR-SPLIT Optional Parameter for STIS . ... DIFFUSE-CENTER Optional Parameter for STIS . ... GAIN Optional Parameter for STIS . ... Position . ...

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• Python: module shelve

. Next: Edition of the Up: Typical Run Previous: Creation of the . All of the atomic data listed in 13.2.1. are needed by the program and are to be entered via this table. A template can be found in MID_CLOUD: ABSP.TBL . The quoted parameters are from Morton and Smith (1973) and according to the author the wavelengths are: . vaccum for 2000 ?, air for 2000 ? . Command: . The actual format of this table is described in section Auxiliary Data. Pascal Ballester . Tue Mar 28 16:52:29 MET DST 1995

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• Permanent telescope parameters
• Parameter estimation
• Order definition: Method Hough

... Classes . ... casa . casa::ObjectPool< T, Key > . ... get (const Key key=Key()) . ... The default key and stack, and the last referenced one (for caching purposes). ... template<class T, class Key> . ... Create the pool. template<class T, class Key> . ... Delete the pool. template<class T, class Key> . ... Decimate the stacks and remove any map entry that is completely unused. template<class T, class Key> . ... const Key . ... Get the object stack for the given key. template<class T, class Key> . ...

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• casacore: casa::FunctionOrder< T > Class Template Reference
• ccontsubtract CentralProcessor 0.11 documentation
• Parameter Set CentralProcessor 0.11 documentation

This page will contain definitions (and basic references) of the following parameters: . cross-sections C ext , C sca , C abs , C bk ; . efficiencies Q ext , Q sca , Q abs , Q bk ; . ... TE/TM mode definitions for arbitrary shapes. Note that some parameters are defined in a quite different (specific) manner than for spherical scatterers, and some definitions in the book of Mishchenko et al. ...

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• Database of Optical Properties -- Level: database

Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents . The parameter file contains information for CONSTRICTOR on the location of the raw data files, start and stop times, integration time, etc. ... The parameter file, YYYY-MM-DD.par , can now be created using the rawlist procedure of . ... Check beginning and tail of the listing for each file. ... Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents Christian Hummel 2015-04-28 ...

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• Stellar parameters from calibrations of spectral types
• OLAS integration test suites
• Score reports

Stellarium 0.12.3 . ... FileљStructure . ... SphericalRegion . DrawParams . ... SphericalRegion::DrawParams Struct Reference . Parameters specifying how to draw a SphericalRegion . More... #include < StelSphereGeometry.hpp > . DrawParams (class StelProjector *projector) . Construct DrawParams with default parameters and specified projector. ... Do not subdivide the region to follow projection distortions. ... class StelProjector * SphericalRegion::DrawParams::projector_ . ...

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• Stellarium: SphereParams Struct Reference
• Stellarium: StelGeometryBuilder Class Reference
• Stellarium: TextParams Struct Reference

spaceweb@oulu.fi - last update: 1 July 1998, 1200 UT (RR) . ... Relates the wave number k to the wave frequency. ... From the equation of motion , m d v /dt = q( v x B ) one can calculate that, in a presence of magnetic field B , a charged particle is accelerated in direction perpendicular to both v (perp) and B . ... The angle a between magnetic field B and velocity vector of a charged particle, v ., i.e., sin a = v(perp) / v(total), where v(perp) refers to the velocity component perpendicular to B . ...

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• Dispersion relation [Oulu]
• Influence of onboard events onto spin parameters
• AZ Key parameters, 1998

... Tte tables of ionosphere and plasmasphere parameters are contained in a file param.tbl. ... Latitude Longitude Numbers of tables for (degree) (degree) Month Wm=10 Wm=100 Wm= 150 80 30 March 1 - 3 397-399 793-795 80 150 March 4 - 6 400-402 796-798 80 270 March 7 - 9 403-405 799-801 60 30 March 10 - 12 406-408 802-804 60 150 March 13 - 15 409-411 805-807 60 270 March 16 - 18 412-414 808-810 40 30 March 19 - 21 415-417 811-813 40 150 March 22 - 24 418-420 814-816 40 270 ...

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• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fo E
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/f min
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fb Es

... This section will deal with obtaining photons within specified regions of an image. Available regions are: Annulus Box Circle Ellipse Field -- entire field Irregular region based on intensity of map... i.e. region defined by contour levels. ... The imcnts task in the xray-spatial package sums the source and background counts in specified regions, and subtracts one from the other properly normalized. ... imcnts* - Find counts in an extended region, after removing an embedded point source . ...

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• Structure of the Spectral Package
• Parameters
• *imexamine* - General analysis of image containing many sources

... Apache HTTP Server Version 2.4 . ... macro_module . ... These macros have parameters. ... macro definition within a <Macro> section, following the apache style. user defined names for the macro and its parameters. macro names are case-insensitive, like apache directives. macro parameter names are case sensitive. macro parameters must have distinct names. error on empty parameter names. redefining a macro generates a warning. macro definitions can be nested... (but what for?) . ... Use of a macro: . ...

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• Program parameters
• mod_session_crypto - Apache HTTP Server
• Kernel tunable parameters

... SGML . The text/html content type . In this section, we begin the specification of HTML 4.0, starting with the contract between authors, documents, users, and user agents. ... These recommendations are not normative and conformance with this specification does not depend on their realization. ... An HTML document is an SGML document that meets the constraints of this specification. ... A user is a person who interacts with a user agent to view, hear, or otherwise use a rendered HTML document. ...

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• On SGML and HTML
• Tutorial on Fortran 90, Digital UNIX
• Dynamic HTML in Communicator

... Measurements Definition Sample Timestamp Definition : Time and date of measurement XML parameter : mtSampTime Windspeed Definition : 3 second rolling average of 250 millisecond samples XML parameter : mtWindspeed Units : MPH Raw Wind Direction Definition : 3 second rolling average of 250 millisecond samples XML parameter : mtRawWindDir Units : Degrees Adjusted Wind Direction ... XML parameter: mt60MinWindGustTime_2 Units: date and time ...

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• http://www.naic.edu/~phil/hardware/weatherstation/parameterDefinitions.pdf
• http://www.naic.edu/~tghosh/software/yfit.pro
• Rotang - IDL procedure for calculating the optimum rotation angle for ALFA

... Files . ... tcc.msg.formatObjFields Namespace Reference . ... Definition at line 36 of file formatObjFields.py . ... Definition at line 107 of file formatObjFields.py . ... Definition at line 115 of file formatObjFields.py . ... Definition at line 129 of file formatObjFields.py . ... Definition at line 122 of file formatObjFields.py . ... Definition at line 213 of file formatObjFields.py . ... Definition at line 139 of file formatObjFields.py . ... Definition at line 247 of file formatObjFields.py ....

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• lsst.coordConv: coordConv::PVTCoord Class Reference
• lsst.tcc: tcc.parse.getCoordSys Namespace Reference
• lsst.coordConv: coordConv::OtherCoordSys Class Reference

Chair of solid state physics . ... Laboratory practical training on the structural analysis for 3rd year students of the Solid State Physics Chair of MIPT . ... X-ray diffraction methods in materials research . Debye method: determination of lattice parameters, identification of crystal phases . ... X-ray phase analysis: computer processing of X-ray diffraction spectra, identification of crystal phases using ICDD database . ... X-ray powder diffraction: qualitative phase analysis. ...

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In this chapter we will consider two very simple but useful Web agents that I have written on Actor Prolog for my own needs. ... Let us start the Web agent. Fig. ... Start of the Web agent. The Context diagram consists of three blocks: "Logic Programming Sites", "Edit", and "Check". ... Some Web sites that are linked with the logic programming and Prolog are listed in the pulldown list (these addresses are transferred to the "Edit" block from the "Logic Programming Sites" block). ...

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• Actor Prolog. Programming language definition.

The data in the Table on p. 5788 – 5789 embrace estimated parameters for 128 binary systems in near Earth, Mars crossing, main belt and Trojan orbits (more than 90% of corresponding objects are marked in the Table "Minor planet lightcurve parameters" as undoubtedly binary and in other cases as suspected binary). ... The data were presented by P. Pravec (Astronomical Institute, Academy of Sciences of Czech Republic) (see Pravec, P., Harris, A. W., 2007. Binary Asteroid Population. ...

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• Table of Minor planet lightcurve parameters
• Parameters of lightcurves of minor planets

tranback -- Transform an X,Y position from output to input pixel position using the same conventions as drizzle tranback xout yout . xout = 400 [real] . ... The X dimension of the input image (this is used to determine the centre which is the origin of the transformations). (nyin = 800) [real] . ... If "output" the input image center is mapped to the center of the output grid, rotated about that center and then shifted along the grid of the output image. ...

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• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)
• SLITLESS (Oct97) --- ST_ECF --- SLITLESS (Oct97)
• MAKEASN (Nov98) --- nictools --- MAKEASN (Nov98)

... spectrum . ... nsource <n> : choice of source function (def: 3=Feautrier) . noptype <n> : choice of continuous opacity (def: 1=Kiel) . nhedat <nhedat> : choice of HeI data (BCS or Mon treal) (def: 1=BCS) . ... read_model <filename>: read model atmosphere in QUB/STERNE2 format . ... wavmax <w_max> : distance from line centre to compute . ... nvturb <n vt > : number of points in -dependent v turb . ... tau_exp <n> : increase resolution of optical depth scale by adding additional points . ...

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• FFIT - Command Syntax
• Sfit Control Language: Classified Listing
• sfit help file

Shell scripts can act like standard UNIX commands and take arguments from the command line. Arguments are passed from the command line into a shell program using the positional parameters $1 through to $9 . Each parameter corresponds to the position of the argument on the command line. ... For example: cat printps # This script converts ASCII files to PostScript # and sends them to the PostScript printer ps1 # It uses a local utility "a2ps" a2ps $* | lpr -Pps1 printps elm.txt vi.ref msg . ...

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• Security Considerations