As it is in Ephemerides task, O–C can be calculated with different accuracy. ... It presents three modes of accuracy. One can calculate position of a minor planet by the formulae of elliptic motion starting from the fundamental set of elements for given minor planet. ... Also there is possibility to calculate positions taking into account perturbations from different sets of perturbing bodies by numerical integration ( Integration mode). ... Accuracy of integration is equal to 10**(–10) AU. ...

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... The procedure of radiometer signal integration can be considered as a sort of reducing dimension of the initial sampling space, where the samples are the result of analog-to-digital conversion. ... The probability distribution of the signal and spikes is completely known. ... The quality of the considered algorithm could be also illustrated by Figure 2 . ... One could see the considered adaptive algorithm is preferable even by low degree of compression, because all spikes have been depressed. ...

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XMM-Newton Science Analysis System . omfchain (omfchain-1.22.13) [xmmsas_20030110_1802-5.4.1] . Meta Index / Home Page Mod-8 noise may affect the estimation of background and the output light-curves of very bright source. An algorithm to account for this pattern around bright objects needs to be developed. ... XMM-Newton SOC/SSC -- 2003-01-10 ...

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• Effects to be Considered
• Algorithm
• XMM-Newton SAS: Watchout Page

... Up: Algorithms . ... The imaging problem can be described as an optimizing problem in mathematics. ... Computer simulations of rotating modulation collimator imaging show that the quality of images from this method is better than that from the traditional cross-correlation method. ... The imaging problem is: . ... The results show that this algorithm can be used in the imaging problem and usually results in a better image than that obtained from a traditional method such as cross-correlation. ...

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• Modelling Spectro-photometric Characteristics of Nonradially Pulsating Stars
• An Integrated Procedure for Tree N-body Simulations: FLY and AstroMD
• A New Stable Method for Long-Time Integration in an N-Body Problem

The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...

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• Anomalous diffraction approximation (AD)
• Linear polarization: wavelength dependence
• Current state

... The evolution of a binary system is considered as a sequence of stages the duration of which are defined by the shortest evolutionary time-scale of one of the binary components (see the list of the evolutionary states of stars in Sections 3 and 4). ... Then the code finds a new stage the binary should transit to, with this stage being determined by the evolutionary states of both components, and calculates it. ... However, one can use the algorithm described above to model their evolution. ...

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• Effect of sources evolution on
• Seminars
• The COOC Criterion (Criterion of Observations versus Calculations)

... P2PP V2.4beta1 Integration Test Report SuSE 7.3 . ... OS : SuSE 7.3 . ... P2PP account(s) : 1797, 1901 . ... All standard testcases have been run on SuSEE 7.3, not new specific bug has been found. Count of testcases entirely executed . ... Total specified testcases . ... Be aware: this is a cumulative count considering ALL different platforms used for this testing. ... Failed testcases count . Failed testcases list . ... 1.3/ . ...

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• DFS commissioning: integration acceptance meeting
• AB structure
• VLTI Calibrator Selection Help Page

... The dynamics of silicate and graphite particles with radii of (0.1-2) 10 -5 cm in the vicinity of the Milky Way is considered. The equation of motion of dust grains is integrated with gravitational attraction, radiation pressure, gas drag, and dust destruction taken into account. The effect of other factors on the motion of grains are discussed. ... Dust is swept out of the Galaxy by radiation pressure from stars at a rate of 0.04 M o yr -1 . ...

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SKA ­ TDT Group On Phase Computation during Folding C.Baffa, E.Giani January 2014 The last part of pulsar search algorithm, as in the SKA TDT group approach, is the verification and optimization of pulsar parameters candidates identified in the previous phases. ... As the phase errors are expressed as fractions of the full period (in our case 44 measurement of 50 s), it is evident that the maximum integration time compatible with single precision phase computation is very short. ...

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• mod_expires - Apache HTTP Server
• The Arcetri Spectral Code - E.Landi and M.Landini (1998)
• The Arcetri Spectral Code - E.Landi and M.Landini (2002)

We call expert systems that implement visualization of decision making procedure with the help of graphical diagrams the visual expert systems. ... Actor Prolog is a powerful instrument of rapid prototyping and programming of visual expert systems, thanks to means of visual programming and graphical user interface development automation based on the SADT diagrams. ... Note that the program has colored the "Prepare berries and fruits" and "Boil berries and fruits with sugar" blocks red. ...

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• Getting Started in Actor Prolog. Oil Production.

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... The algorithm and appropriate program for decametric radiosignal propagation conditions prediction for paths from 500 to 9000 km have been developed at ISTP SB on the basis of normal wave method (AltyntsevaB.I,Iliyin N.V., Kurkin V.I. and others //Decameters channel simulation on the base of normal wave method . ... Solar activity indices are chosen automatically from the prediction date from the database . ...

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• East Siberian Center for the Earth's Ionosphere Research. VS data on-line

Program: MOMENTS Purpose: Program to calculate moments and other properties of a profile Category: MANIPULATION, CALCULATION, PROFILES File: moments.c Author: M. Vogelaar Keywords: INSET= Give set (, subsets): Maximum number of subsets is 2048. ... 3: Physical coordinate of peak value in profile. ... If there are a certain number of adjacent subsets with amplitudes within the given range, and this number of subsets is greater than or equal to WINDOW, these sub- sets are taken into account. ...

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• moment
• Preprocessing for Selavy CentralProcessor 0.11 documentation
• Errors associated with reducing filterbank data

... The experience of determination of the link between radio sources and dynamical reference frames is presented. To obtain this connection we used a series of very long baseline interferometry (VLBI) observations of the spacecraft Phobos-2 and angularly nearby quasars. ... The dynamical reference frame is determined by equator and equinox of these ephemerides. ... References . ... The relative orientation of the radio and dynamical reference frames can be described by a sequence of three rotations . ...

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• A Calculation of derivatives
• OptInt PmWiki : MROIFastTipTilt / Tech Meet 7
• An expanding plasmon model for the radio outbursts of Cir X-1

... Since image restoration algorithms are highly sensitive to the accuracy of the calculated PSF, a significant portion of our research effort is devoted to accurately modeling the PSF which is a highly non-linear problem. Our approach is based on analytical modeling of the wavefront phase using Zernike polynomials. ... In the Fourier domain, we scale the phase map by an observed PSF to more accurately account for the HST/FOC combination. ... The final result is an improved estimate of the phase map. ...

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• Update to the dark rates of the COS FUV segments and impact on ETC calculations
• ACS Instrument Handbook for Cycle 20
• Space Telescope Imaging Spectrograph Instrument Handbook

Geomagnetic storms and substorms are a natural hazard similar to hurricanes, floods etc. ... Solar and geomagnetic activity also probably influences the Earth's climate and human health. ... Under southward directed IMF the Earth's magnetosphere is open to input from the solar wind flow. ... Since practical importance of solar wind measurements was recognized, a number of approaches was developed for prediction of the geomagnetic activity basing on the solar wind data. ...

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• The INTERBALL Tail PROBE orbital elements
• The INTERBALL Auroral PROBE orbital elements
• Space Research Institute (IKI) Seminar

AO Home AO Astronomy Robert Minchin Blog Publications IDL Routines . Rotang can either be run from the command line as described here or through the alfa_ang GUI . ... To run rotang at Arecibo: . Start IDL . ... Run Rotang: . rotang, Date , RA , Dec , Time , /choice . ... Rotang also calculates the Azimuth and Zenith Angle fir every source. If the Zenith Angle is greater than 20 degrees, then the program will return that the source is down and will not calculate an optimum ALFA angle. ...

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• INTRODUCTION to Spectral Line Observing at AO
• Alfa_ang - IDL procedure for calculating the optimum rotation angle for ALFA
• Spectral-Line Observing

Next: *upspecrdf, downspecrdf* - Transform Up: Spectral Analysis Previous: *grid_plot* - Plot Results . The conversion of count rate to flux depends on the intrinsic spectrum of the source, so xflux must be used in conjunction with fit . Fit generates a table of the best fit intrinsic spectrum ( _int.tab extension). xflux uses this table to calculate either the integrated flux between two energy limits or the flux density at a specific energy. ... This produces ``..._obs.tab'' file. ...

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• Funtools and DS9 Image Display
• Home Page for SAOimage: The Next Generation
• The AstroStat Slog Blog Archive Line Emission [EotW]

Hide Zen home . ... GiST . ... It could be considered as ancestor of "Relational Extenders" in DB2, Cartridges in Oracle and DataBlade in Informix. extending and improving of GiST interfaces to make easier developing GiST based extensions and implementation of ADT not supported by current implementation of GiST core. ... Figure out how to configure parameters to GiST index supported functions, for example, change size of signature SIGLENINT for tsearch2 index, which could greatly improve performance. ...

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• Zen: NewExtentsBasedRanking
• Zen: tp search en
• Jenam 2000

M1 image More About M1 Nice Color Picture . ... M16 image More About M16 HST image . ... M31 image More About M31 Nice Color Picture . ... M42 image ; M43 image More About M42/43 Nice Color CCD Picture . M51 image More About M51 Color Image of M51 M51 Supernova . M57 image More About M57 Nice Color CCD Picture Very Deep M57 Image . ... M81 image More About M81 M81 Supernova Ultraviolet Image of M81 More about Ultraviolet Imaging . M82 image More About M82 M82 False Color M82 True Color . ...

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• Astronomy HyperText Book

... The described algorithm is suitable for measurements of complex images of stars. ... a) the zero-based number of stars in the complex (multicentric) image, . b) set of preliminary coordinates - x i , y i , for all stars, index i is number of a star, . ... i - index of a star in the complex image; . ... These parameters are calculated by a nonlinear method of a least squares.The main output parameters of this algorithm are x i , y i ; where the index i is number of a star in the multicentric image. ...

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