System parameters on Digital UNIX . ... Digital and Cray use the number of bytes as the KIND -parameter. ... LOGICAL Default byte word KIND number = 4 1 4 LOGICAL Default double quad KIND number = 4 8 16 INTEGER int15 int31 int63 KIND number = 2 4 8 digits = 15 31 63 radix = 2 2 2 range = 4 9 18 huge = 32767 2147483647 9223372036854775807 bit_size = 16 32 64 REAL single double quad KIND number = 4 8 16 digits = 24 53 113 maxexponent = 128 1024 16384 minexponent = -125 -1021 -16381 ...

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• Specifications
• The new precision concept
• NAG's Fortran 90

Next: CAL_getBoresightMatrix Up: Routines of the Calibration Previous: List of CCF Components Contents . ... The CAL functions CAL_getBadPixelList & CAL_getBadPixelMap use the CAL state variable temperature only to check that the current operating temperature is consistent with the CCF constituent BadPix . ... Used CAL State Variables . List of CCF Components used . ... Next: CAL_getBoresightMatrix Up: Routines of the Calibration Previous: List of CCF Components Contents Michael Smith 2011-09-20 ...

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• EPIC Related CAL Routines
• OM Related CAL Routines
• Procedure

... A Miriad uv dataset is composed of a collection of items and ` u-v variables'. The variables are parameters that are known at the time of the observation, and include measured data, and the description of the observation set up ( e.g. correlator set up and observing centres). Table B.1 gives a list of the items that are used to build up a Miriad uv dataset. ... integer . ... antenna gain table . ... number of feeds on each antenna . ... frequency set up description table for `bandpass' . ...

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• Determining UV Variables and Their Characteristics
• Direct Access to UV Variables
• User Parameters - Mosaicking Continuum images CentralProcessor 0.11

Fringe parameters are the complex visibility, the squared visibility amplitude, and the total count rate. These can be computed from bincounts using the functions fringevis , fringevissq , and fringenphot . v=fringevis(bincounts(1,*,*,*)) . ... Instead of computing the modulus of the complex visibility, we use a different estimator for the squared amplitude. ... I have verified with simulated fringe frames that this procedure results in the correct squared visibility amplitudes. ...

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• Fringe delays
• Coherent integration
• POLIMODEL (V2.00) --- November00 --- POLIMODEL (V2.00)

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Namespaces . ... NamespaceљList . NamespaceљMembers . ... getPVTList . ... tcc.parse.getPVTList Namespace Reference . ... listљ . ... numAxes , . ... number of axes of PVT data required . ... TAI date (MJD, seconds) to use if time is omitted . ... numValues: the number of values explicitly specified by the user (positions, velocities and TAI, as appropriate) . ... An invalid number of values is seen . ... list tcc.parse.getPVTList.__all__ = ["getPVTList"] . ...

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• lsst.tcc: tcc::tcspk Namespace Reference
• lsst.coordConv: coordConv::OtherCoordSys Class Reference
• lsst.coordConv: coordConv::Coord Class Reference

... Abstract The function returns the ordinal position of any given item in a double precision set. ... Detailed_Input item is a double precision number to be located within a set. set is a double precision CSPICE set that is to be searched for the occurrence of item. set must be declared as a double precision SpiceCell. ... Particulars A natural ordering can be imposed upon the the elements of any CSPICE set, be it integer, character or double precision. ... Link to routine source . ...

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• CSPICE Routines: ORDI_C
• HST Image Restoration with Variable Resolution
• CSPICE Routines: ORDC_C

Next: External Functions Up: Fitting of Data Previous: The Corrected Gauss--Newton . ... Basic functions are either defined in the system or defined by the user as external FORTRAN routines. ... Basic functions are specified by the name, the independent variable(s) and parameter(s), with optional guesses for the parameters, following the syntax: name(var1[, ];par1[, ]) [par1=value] . ... Parameters are defined by unique names after the semicolon in the function specification. ...

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• Parameter estimation
• Values, Variables, and Literals
• DO Loops

Program to demonstrate the Euler method on ! dy/dx = y over the interval [0,1] program euler implicit none integer, parameter :: n = 10 ! ... kind for double precision integer :: i ! loop counter real(dp) :: x, y, h ! ... interval spacing h = 1.0_dp / n ! ... open file for results open(10,file='euler.dat') ! ... close file close(10) contains ! this function provides the value of dybydx at (x,y) real(dp) function f(x,y) real(dp), intent(in) :: x, y f = y end function f end program euler ...

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• http://www.mrao.cam.ac.uk/~rachael/compphys/examples/runge.f90
• OptInt PmWiki : PmWiki / Debug Variables
• OptInt PmWiki : PmWiki / Markup Expressions

... In order to disentangle the effects of different climate variables on tree-ring growth rates of different species, and to explore the possibility that more than one species could improve the accuracy of the reconstructions of climate using tree rings, a methodical study of trees in close proximity to the Armagh Observatory climate station was initiated together with Ana Maria Garc?a Su?rez, and continued as part of the latter's PhD thesis with John Butler and Professor Mike Baillie (QUB). ...

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• SCL Sfit SYN Commands
• Armagh Observatory
• SCL Sfit Genetic Commands

... astro-ph . ... Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . ... Quasar Variability in the Framework of Poissonian Models . ... It is shown that in this very general framework the well established anti-correlation between variability amplitude and wavelength can only be understood as an effect of an underlying spectral component which remains stable on long time-scales, and is redder than the variable component. ...

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

... We have compared visualized fields of GSC and USNO A1.0 catalog with unpublished photographic finding charts that were sent by L. Plaut to the compilers of the GCVS. ... 7-15 A9 --- GCVS GCVS or NSV name 17-25 F9.4 --- GSC GSC number 26 A1 --- NoteFlag *Nonstar (GSC) flag 28-29 I2 h RA2000GSC.h Hours RA (GSC), equinox 2000.0 31-32 I2 min RA2000GSC.m Minutes RA (GSC), equinox 2000.0 34-38 F5.2 s RA2000GSC.s Seconds RA (GSC), equinox 2000.0 40 A1 --- DE2000GSC.- ... Plaut, L., 1966, Bull. ...

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• General Catalogue of Variable Stars: Homepage.
• General Catalogue of Variable Stars: Vols I-III (the new electronic version).
• General Catalogue of Variable Stars: Description

... we show that the comparison between the calculated and observed numbers of the most ``fragile'' (from the point of view of the binary evolution scenario )   galactic binary types (such as X-ray low-mass X-ray binaries (LMXB), cataclysmic variables (CV),   Be-stars   with compact companions, relative number of visible binary radiopulsars   with normal and compact secondary components) impose certain constraints on the feasible initial ... Phenomenological Kick Velocity . ...

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• Periodic radiosource LSI+61 303
• The Model
• Transparency of the Stochastic Background

... Characteristic parameters of subsystems RR Lyrae field stars and globular clusters . ... RR Lyrae . ... 0.05 . ... lim R max , kpc . ... Z o , kpc . ... grad R [Fe/H], kpc -1 . ...

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• RR LYRAE VARIABLES SUBSYSTEMS IN THE GALAXY, figures
• Vladimir Marsakov Abstracts

. На главную страницу НМУ . [ Postscript (20K) | Zipped postscript (8K) ] . Голоморфные функции и отображения. Феномен Хартогса. Оболочки голоморфности. Голоморфная выпуклость. Многообразия Штейна. Псевдовыпуклость и плюрисубгармоничность. Решение $\bar d$-уравнения по Хермандеру. Топология многообразий Штейна по Элиашбергу и Гомпфу.

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• Dubna-2004: On functions of complex variables
• Complex Analysis
• Conference "Combinatorial Methods in Physics and Knot Theory" (February 2005)

There are some variables which are set internally by the shell and which are available to the user: Name Description . ... 0 the name of the command currently being executed. $# the number of positional arguments given to this invocation of the shell. $? the exit status of the last command executed is given as a decimal string. ... For example '1 2' 3 becomes "1 2 3" . is identical to the arguments received by the shell, the resulting list of words completely match what was given to the shell. ...

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• Rudnitskij Georgij M. Home Page
• Passing arguments to the shell
• Index: P

... 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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• WAPP File Format Page
• Debugging and Tracing

Plasma models and main parameters. ... Magnetic diffusion. ... Double- adiabatic invariants for a plasma in strong magnetic field. One- fluid MHD. ... Frozen-in properties of magnetic field in plasma. ... Force- free magnetic field configurations. ... Dispersion of plasma waves in linear theory. ... Waves in non- magnetic plasma. ... Electromagnetic waves in plasma. ... Dispersion relation for waves in cold magnetized plasma. ... High- frequency electromagnetic waves in cold magnetized plasma. ...

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• A computer controlled low light photometer for nightglow observations
• Additional Parts of Theoretical Astrophysics
• Satellite Data Processing

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: TextParams Struct Reference
• Stellarium: Skybright Class Reference
• Stellarium: StarMgr Class Reference

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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• *tvmark* - Mark pixel positions on the display
• The AstroStat Slog variable selection
• The AstroStat Slog Blog Archive [ArXiv] classifying spectra