... Satellite data ] . SMIS ] . The program is designed to process the specific AVHRR instrument data for calculation and analysis of temperature fields on the sea surface and upper level of clouds. It performs brightness correction for visible channels with regards to clouds altitude. ... The program features a wide variety of classification algorithms (including two-dimensional histogram analysis) and enables to construct personal procedures for classification. ... Back to SMIS Home Page . ...

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Next: stecf.cplucy - Enhanced Two-channel Up: The ``stecf" IRAF Layered Previous: The ``stecf" IRAF Layered . For many years the ST-ECF has developed IRAF tasks and packages for HST and related data analysis. ... To allow wider and more efficient distribution and to bring all components to a uniform level of quality and documentation we have decided to combine these components into a standard-format IRAF package to be called ``stecf''. ...

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• The Stellar Population in the NICMOS Parallel Fields
• CPLUCY (V0.22) --- Sep98 stsdas.contrib --- CPLUCY (V0.22)

... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...

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• Kholtygin Shneiwais, Astrophysics, (2005)
• Polarization properties (transmitted radiation)
• Database of Optical Properties -- Level: subpage

... Wind Baffle Parameters . ... As part of this analysis, the volume, mass, center of gravity and mass moment of inertia of the telescope and optics support structure (OSS) were computed. ... The total moment of inertia of the circular floor panel, wind baffle and telescope in azimuth should be correct to 30% but is dependent on estimates of the mass of equipment supported below and above the circular floor panel. ... Table 8 : Masses and mass moments of inertia of the wind baffle components. ...

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• sgs summary
• Astrophysical Research Consortium - Apache Point Observatory
• lsst.coordConv: coordConv::FK4CoordSys Class Reference

. Authors: V.A. Marsakov , Yu.G. Shevelev , . Journal: Bull. Inform. CDS, 1988, № 35, p.129-130.      The values of [Fe/H], the distancec, the componets of the space velocities and orbital parameters are calculated for 1304 non-evolved F -stars with homogeneous data and proper motions.

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• Vladimir Marsakov Publication List
• Population of Galactic globular clusters, tabl
• Vertical Structure, figures

... According to the most popular cosmological paradigm, the greater part of the galaxy mass is accumulated in the dark matter halo. ... The polar ring galaxies (PRGs) reveal external rings or disks of gas, dust and stars rotating in a plane roughly perpendicular to the disk of the central galaxy. ... The shape of the dark halo in the model was chosen so as to achieve the best fit to the observed rotation of both galaxies themselves and their polar rings. ... The SPRC-7 galaxy. ...

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• Galaxy sector, archive 2014
• Galaxy sector, archive 2012
• Galaxy sector, archive 2006

... Subject and Problems of Stellar Astronomy. ... Plane of Galaxy, Methods of Its Location Determination. ... Stars Distances. ... Other Methods of Stars Distances Determination. ... Tangential Velocities, Their Determination by Self-Motions. ... Determination of Solar Apex and Spatial Velocity by Radial and Spatial Velocities of Stars. ... Features of Orientation and Parameters of Peculiar Stellar Velocities Ellipsoid. ... General and Selective Light Absorption in Galaxy. ... Darc Clouds in Galaxy. ...

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• Extragalactic Astronomy
• Theoretical Astrophysics
• Optical static Fourier spectrometer

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Measured radial velocities for the primary (full symbols) and secondary (empty symbols), phased with the orbital period of 5.9051102 0.0000023 days. ... HD 98088 is a synchronised, double-lined spectroscopic binary system with a magnetic Ap primary component and an Am secondary component. ... The magnetic field in the primary is predominantly dipolar, with the positive pole oriented approximately towards the secondary. ...

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• ffit help file
• Refereed Journal Publications 2004
• Stellar Atmospheres Software

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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• Getting Started in Actor Prolog. Oil Production.
• Getting Started in Actor Prolog. Component-Oriented Programming.

... Предлагается новое направление для анализа пространственно-времен-ных вариаций яркости зеленой короны. ... Бадалян О.Г., Куклин Г.В., Обридко B . ... Бадалян ОТ., Куклин Г.В., Обридко В.Н., Сикора Ю. Динамика режи-мов свечения зеленой короны в циклах 18-22 / Крупномасштабная структура солнечной активности: достижения и перспективы / Под. ред. ... Бадалян О.Г., Обридко В.Н, Сикора Ю. Прогноз 23-24 циклов солнечной активности по данным о яркости зеленой короны // Настоящий сбор-ник. ...

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• Magnetic Flux of EUV Arcades and Dimmings
• Astronomical and Astrophysical Transactions, 2000,
• APEX/Equipment

Peremennye Zvezdy ( Variable Stars ) 33 , No. ... From our comparison of magnitudes of bright stars in the Hipparcos catalogue and in the Tien-Shan catalogue of magnitudes, we compiled a list of stars that could be candidate photometric standards in the northern sky. The selected stars were tested for variability using the technique. ... Fig. ... It follows from Fig. 7 that if , then, according to the theory, we should expect the star to be variable. 54 stars are situated in the range. ... star . ...

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• Astronet > Sky Map, professional edition

... 2009) 0 Fig.1 Ї Max-Planck-Institute for Radioastronomy, Bonn , VLBI ESO, COMPONENTS PARAMETERS FROM INTERFEROMETRY Ї Following S.Kraus et al. ... Using i=105o , we obtain v sini = 32 km/s. BEST MODEL FIT 1OriC 1 Ї Mass, M Ї Luminosity, log L Ї Radius, R Ї Teff, K Ї log g Ї Equatorial rotation velocity, km/s Ї Magnetic field , G Ї The time of life, yrs 35.8 5.20 10.0 37000 4.01 5.4 500-1500 150 000 1OriC 2 10.0 4.69 8.2 30000 3.60 96.2 moves to MS 1 OriC ...

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• http://hea.iki.rssi.ru/integral06/papers/F40_Ziolkowski01-03Mar07_22:49:23.pdf
• http://hea.iki.rssi.ru/integral06/papers/E36_Stephen01-07May07_17:57:56.pdf
• http://hea.iki.rssi.ru/integral06/papers/G32_Fiocchi01-22Dec06_16:28:45.pdf

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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• Solar Wind Conditions
• List of currently available KP AZ.
• Microwave Remote Sensing

... FTP access the basic models is here . ... Below, we put short descriptions of the used SED models for the photometric redshifts providing by the current server . ... The uniqueness of this model consists in expanding to the near IR (NIR) of Rocca-Volmerange and Guiderdoni's (1988) atlas of synthetic spectra with a revised stellar library, which includes parameters of cool stars. ... Homepage of the GISSEL model). ... Another model used earlier is the model of synthetic spectra of Poggianti (1997). ...

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• Methods and results of radio cosmology. Plan.
• Radio Sources Parameters

Bulges and disks in spiral galaxies: Clues for secular evolution? Leslie Hunt INAFIstituto di Radioastronomia, Sezione Firenze Tracing Dust in Spiral Galaxies Ghent 1317 May 2007 Galaxy Hubble types N2775 (SAab) [Frei] N1350 (SBab) [OSU] M51 (SAbc) [NOAO] M100 (SABbc) [Frei] Tracing Dust in Spiral Galaxies Ghent 1317 May 2007 Main structural components: bulge and disk ... Tracing Dust in Spiral Galaxies Ghent 1317 May 2007 What about bars? ...

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• http://www.arcetri.astro.it/igm50/posters_all/pieri.pdf
• http://www.arcetri.astro.it/irlab/doc/library/nr/f14-0.pdf
• http://www.arcetri.astro.it/irlab/doc/library/recipes/bookcpdf/c14-0.pdf

... Exploring the physics of Type Ia supernovae through spectral analysis . ... Their progenitor scenario as well as the details of the explosion mechanism remain a mystery. ... It produces a supernova spectrum for a given luminosity, photospheric velocity, time since explosion and several elemental abundances. Tweaking these parameters to produce a spectrum that fits an observed spectrum is a complex, as of yet, manual task. ... The search space is large and complex. ...

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• Emma Kirby - Science
• GSAOI Bulk Motions Science Page
• GSAOI Component Supplier Links Page

Stellarium 0.12.3 . ... File Structure . File List . ... core . modules . Skylight.hpp . ... 33   float color[3]; // 3 component color, can be RGB or CIE color system . ... 48   void setParams( float sunZenithAngle, float turbidity); . ... 109   float zenithLuminance; // Y color component of the CIE color at zenith (luminance) . 110   float zenithColorX; // x color component of the CIE color at zenith . 111   float zenithColorY; // y color component of the CIE color at zenith . ...

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• Stellarium: SphereParams Struct Reference
• Stellarium: BigStarCatalogExtension::SpecialZoneArray< Star > Class Template
• Stellarium: TextParams Struct Reference

... Moscow, Russia . ... March-October 2000 . ... Gusev A.S. Multicolor CCD Photometry of Six Lenticular and Spiral Galaxies. ... Gusev A.S., Park M.-G. Structure and stellar population of ringed barred galaxy NGC 2336 // Astronomy and Astrophysics, 2003, V.410, P.117-129. ... Gusev A.S. Photometric Properties of Bars in Galaxies // Astronomy Reports, 2000, V.44, N9, P.579-591. ... Gusev A.S. BVRI CCD Photometry of Pecular Galaxies NGC 5605 and NGC 5665 // Astronomy Reports, 2000, V.44, N9, P.569-578. ...

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• IDL programs
• Data bases of Natural Satellites. Documentation. Structure
• Speckle polarimeter

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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• LPCBC: Abstract 2_35
• III International Astronomy Olympiad, Problems to solve
• Equipment LSR ISSP RAS

Preliminary results of astroclimate parameters measurements at the Sternberg 2.5m telescope installation site V.Kornilov, N.Shatsky, S.Potanin, O.Voziakova, B.Safonov Moscow, 2008 Acknowledgements A.Belinskiy M.Kornilov A.Tokovinin M.Kuznetsov P.Kortunov E.Gorbovskoy SAI administration some SAI students Pulkovo solar station (KHSS) staff RFBR support MAVEG Gmbh Why to study optical turbulence and some other relevant ... Mean seeing by DIMM data for this night is 1''5. ...

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• . The . MASS . Group .