Next: Regularization of Van Up: Deconvolution Previous: Tikhonov's regularization and . If we use an iterative deconvolution algorithm, such as Van Cittert's or Lucy's one, we define , the error at iteration n : . ... The wavelet coefficients provide a mechanism to extract from the residuals at each iteration only the significant structures. ... is the standard deviation of the noise at scale j , and is a function which is defined by: . ... Regularization of Van Cittert's algorithm . ...

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• Regularization of Van Cittert's algorithm

... We describe a parallel code for 3-D structure detection and morphological analysis. The method is based on a multiscale technique, the wavelet transform and on segmentation analysis. ... This paper presents a new parallel code, that allows a rapid structure detection and morphological analysis in a 3-D set of data points. ... Segmentation analysis. ... Our code is based on the programming paradigm MASTER/SLAVE . ... Finally, the morphological analysis is executed by the master. ...

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• Spatial Structure of NGC 6822: An Example for Statistical Modeling of
• Positive Iterative Deconvolution in Comparison to Richardson-Lucy Like
• A New Field-Matching Method for Astronomical Images

This home page belongs to small group of scientists working at . Sternberg Astronomical Institute which is a part of Moscow State University . ... Электронная библиотека научно-технической и художественной литературы (доступна только из ГАИШ) . ... Local staff . Dr. Edward Kononovich (konon -at- sai.msu.ru), Associate Professor . ... Dr. Sergey Ayukov (asv -at- sai.msu.ru), Research Fellow, Webmaster of the group . ... Joint seminar of Solar Studies Structure Group and Solar Photometry Group . ...

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... Development of Ideas of Structure and Evolution of Stars. Integral Features of Stars, Which Determine Their Structure, Direction and Rate of Evolutuion. ... Connection between Potential and Thermal Energy of Star. ... Structure of a Main Sequence Star. Features of Massive Stars Evolution on the Main Sequence. Internal Structure of the Sun. ... White Dwarfs, Their Features. ... Evolution from the Main Sequence of Massive Stars. ... Evolution of Small Mass Stars till White Dwarfs Sequence. ...

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• Introduction to Space Gas-Dynamics
• Physics of Heliosphere
• Solar Physics

... This is done by incorporation of the inverse weighting matrices and into the quadratic error term . The Toeplitz matrix determines a linear shift invariant regularization function: . ... Application of matrix differentiation rules and some matrix algebra show that the diagonal elements of the optimal diagonal matrices must be equal to the diagonal elements of the previously determined optimal general weighting matrices so that . ... is estimated from the measured data. ... Therefore we estimate: . ...

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• Introduction
• Adaptive Regularized Restoration Algorithms Applied to HST Images
• Iterative Image Restoration

... Another significant contribution to the crystal energy of metals is the electron-ion interaction or the electron bandstructure energy (E BS ) which is defined by the interaction of valence electrons and the Brillouin zone (BZ) planes. ... The program BRIZ has been developed for 3D visualization of Brillouin zone configurations and intersections of BZ planes with a Fermi sphere[4]. ... 1.75 (electrons/atom). ... 4] Degtyareva V.F., Smirnova I.S.: BRIZ: a vizualization program for Brillouin zone ? ...

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• Laboratory for Spectroscopy of Molecular Structures
• Department of Solid State Physics MIPT
• Laboratory of Real Structure of Crystals ISSP RAS

GiST home | Introduction | ... GiST is a height-balanced tree structure with tree nodes containing (p, ptr) pairs, where p is a predicate ( attribute ),which is used as a search key, and ptr is the pointer to data for a leaf node or a pointer to another tree node for a non-leaf node. ... Every node contains between min and max index entries unless it is the root . ... For each index entry (p, ptr) in a non-leaf node, p is true when instantiated with the values of any tuple reachable from ptr . ...

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• Introduction to The Web Nebulae
• Zen: SkyPixelization
• APOD: 2013 May 19 - Earths Richat Structure

Next: Model of clusters Up: paper2 Previous: paper2 . ... It allows estimating different microphysical properties of scatterers (size, complex refractive index, shape, etc.) from measured characteristics of the scattered radiation. ... The complexity of the direct problem depends on its input parameters characterizing the shape, size and structure of the scattering particle. ... Next: Model of clusters Up: paper2 Previous: paper2 root 2003-04-11 ...

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• Vladimir P. Reshetnikov's Home Page
• Wavelet references
• LPV and Wind structure of OB stars

ATNF engineering research programs focus on developing, and applying, new technology and advanced design techniques to radio astronomy and allied fields. ... There are three groups within the ATNF engineering structure: . ... This project, designed to allow rapid alternation between radio astronomy and spacecraft tracking modes, was undertaken in collaboration with outside consultants and received an honourable mention in the the 1997 Institution of Engineers (Australia) awards program. ...

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• Research - Structure formation in the Sculptor Group
• Contents
• Large Scale Structure of Orion

Next: Armagh Planetarium Up: Introduction Previous: Vision Contents . The Armagh Observatory and the Armagh Planetarium are distinctive organizations, part of a single corporate entity ``The Governors of the Armagh Observatory and Planetarium '' described in The Armagh Observatory and Planetarium ( Northern Ireland ) Order 1995, which superseded the original 1791 Act of the Irish Parliament entitled ``An Act for Settling and Preserving a Public ... Armagh Planetarium . ...

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• Introduction
• Explosive Events
• Vision

... The file names' construction . The flight (m) stage's file set . ... the orbital data used for the flight operation monthly (m) long-term planning, . ... The orbital calculations are based on the initial orbital data determined by KIAM RAN using the orbital radio- measurement treatment. The determined initial orbital data are presented as a state vector (satellite position and velocity) in the J2000 reference. ... Accept the file with extension '.bgr', where the Moscow time (MT=UT+3h) is used. ...

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• Space Research Institute (IKI) Seminar
• Brief History Introduction Brief History Introduction
• IKI structure

The HyperNews Linux KHG Discussion Pages . Forum: Tour of the Linux kernel source . Keywords: configuration makefile . Date: Wed, 22 May 1996 17:34:39 GMT . From: Steffen Moeller < steffen@di.unito.it > . ... Or is this too trivial for a Hacker's Guide? ... If there's some positive feedback I'd like to start on this myself, but I'd need some help - at least for the language. ... Editing services available... by Michael K. Johnson . ... Kernel configuration by Venkatesha Murthy G. ...

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• The Sun: a Pictorial Introduction
• Ray Structure - Halley's Comet
• How can my device driver access data structures in user space?

... 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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• Laboratory of spectroscopy and photometry of extragalactic objects : Vortex
• LWN: Using read-copy-update
• Introduction

... The axial support is provided by 78 air pistons. ... The transverse support is provided by 38 air pistons, supported by cantilevers from the mirror cell, that act on the mirror local center of gravity surface. ... The locations where the transverse mirror support forces should be applied to the mirror are listed in Table 1 and illustrated in Figure 1. ... Figure 1: CAD drawing showing the 2.5-m primary mirror and the locations of the transverse support posts (black) and axial pneumatic pistons (blue...

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• MILT Multiple Instrument Large Telescope
• Telescope Parameters

Proposal Identification No.: A2220 Date Received: 2006-Feb-15 15:25:40 Technical Page Proposal Type: General Category: Sub-Category: Observation Category: Total Time Requested: Prop osal Title: ABSTRACT: Regular Astronomy Spectroscopy Galactic 42.5 Hours Interfaces in the ISM: Mapping a Cold Cloud Boundary With GALFA we mapped part of the coldest HI cloud known. ... Three years ago in the pre-ALFA era boundary of this sheetlike cloud. ... Part of the observing run. ...

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• Galactic Spiral Structure in H I Emission and Self-Absorption
• Introduction
• I-GALFA Survey Introduction

... The HH flow associated with young stellar object HL Tau has an exciting history and even until now the origin of some its features is not clear yet. ... Knotty structures of Herbig-Haro jets are common phenomena and knowing the origin of such structures is essential for understanding the processes of jet formation. ... In the flow detected compact knots with high (-150 km/s) and bow shape structures in front of those, with low radial velocities (-50 km/s). ...

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• Observatory structure
• New data on the cpmplex field structure of chemically peculiar stars
• Structure

... V.V.Shevchenko, Sternberg State Astronomical Institute, Moscow University, Universitetsky 13, Moscow 119899, Russia, shev@sai.msu.ru . ... 1.Sternberg State Astronomical Institute, 119899, Moscow, Russia. shev@sai.msu.ru . ... V.V.Shevchenko, Sternberg State Astronomical Institute, Moscow University, Moscow 119992, Russia, shev@sai.msu.ru . ... 119992 Moscow, Russia; . ... 2Sternberg Astronomical Institute, Moscow University, Moscow, 119992, Russia, . ... Moscow, 119992, Russia shev@sai.msu.ru . ...

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• Svetlana G. Pugacheva

... Imaging of the core of the OMC-1 region using NICMOS camera 2 through the F212N and F215N filters shows a wide variety of interesting structure on scales of 0.2" at a very high dynamic range (Stolovy et al. ... The application of image restoration techniques, including multi-channel variants of the Richardson-Lucy technique, offers the chance to enhance structure on the finest scales and also to suppress the prominent and richly structured point-spread functions of the many bright stars in the...

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• The Structure and Composition of High Redshift Radio Galaxies
• stecf.cplucy - Enhanced Two-channel Photometric Restoration

... Doug's Home Page . ... S-Lang structures are converted to hash references in Perl , as shown below. ... n\n ; print Structure contents:\n ; # you can treat $s as a reference to a hash array in most respects, except: # - the order of the keys in the array matches that of the # original S-Lang structure # while ( my ( $ key , $ value ) = each %{$s} ) { print key $ key \t has a value of $ value \n ; } print \n ; $$s{afield} = 'a changed field value '; print ...

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• Vertical Structure of the Secondary: Hydrostatic Model
• Martin Elvis - Home Page
• The AstroStat Slog DEM

Next: Transparency of the Stochastic Up: Model of the Galaxy Previous: Frequency distribution of galactic . ... The parameters of the model resulted from a numerical fitting of various data, such as the observed distribution of the young star population and neutral hydrogen, the density of population II stars in the vicinity of the Sun, the galactic rotation curve and the dynamics and distribution of globular clusters   and dwarf irregular satellites of the Galaxy. ...

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• Accretion Mechanizsm of the Formation of the Large Structure
• Lectures and presentations
• Introduction