What's new at the DOP? ... What is in the database? ... i) original codes realizing different methods to calculate the optical properties of non-spherical (inhomogeneous) particles; . ii) reviews of exact and approximate methods of light scattering theory ; . iii) a database of several tausends references to papers on various aspects of light-scattering theory and its applications; . ... vi) a self-training algorithm of determination of the optical properties of fractal-like clusters; . ...

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• Database of Optical Properties -- Level: database
• Database of Optical Properties -- Level: subsubpage
• Database of Optical Properties -- Level: subpage

Instrument Summary -- Why Use the GHRS? Here we provide a brief overview of the basic properties of the GHRS. ... The GHRS can obtain spectra from about 1150 to 3200 . ... The repeatability of fluxes is even better, being better than 1%; i.e., it is possible to compare measures of the same wavelength in the same star at different times to within 1% for observations with the LSA. ... The source to be observed may be placed in a Large Science Aperture (LSA) or a Small Science Aperture (SSA). ...

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• Spitzer SAGE-SMC Infrared Photometry of Massive Stars in the Small Magellanic
• ACS Instrument Handbook
• Space Telescope Imaging Spectrograph Instrument Handbook

... X-ray (left) and magnetic field (right) evolution of an X-ray jet in coronal hole. ... In both coronal holes and quiet-Sun regions, all brightening events are associated with bipolar regions and caused by magnetic flux emergence followed by cancellation with the pre-existing and/or newly emerging magnetic flux. ... The dominant flux of the coronal hole form the largest concentration of magnetic flux in terms of size while the opposite polarity is distributed in small concentrations. ...

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• Online materials for the coronal holes brightening events paper
• STELLAR PROPERTIES
• Atmospheres

Proposal Identi cation No.: P1877 Date Received: 2004-Oct-01 23:28:48 Technical Page Proposal Type: Regular General Category: Pulsars Observation Category: Total Time Requested: 9 Hours Proposal Title: ow-frequency millisecond pulsar polarimetry ABSTRACT: We request 9 hrs of observing time to investigate the emission properties (spectral behavior, intensity-pro le complexity and polarization) of a small sample of millisecond pulsars (MSPs) at 327 MHz. ... Maybe X Part of the observing run. ...

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• Heiles Symposium Presentations
• Incoherent scatter
• HISA Poster for the 197th Meeting of the AAS, January, 2001

... This image was made when the spacecraft approached to within 18 miles of Deimos' surface. ... Launched on January 6th, NASA's Lunar Prospector spacecraft has been exploring the Moon with instruments designed to sense global properties while orbiting pole-to-pole, 63 miles above the lunar surface. ... Recent data from the Galileo spacecraft currently orbiting Jupiter now confirms that these rings were created by meteoroid impacts on small nearby moons. ... Dust Hip Deep on Phobos . ...

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... The Science Operation Department is composed of Astronomers, Telescope Instruments Operators(TIOs) and Data Handling Administrators(DHAs). ... Astronomers have proposed several methods to quantitatively measure the amount of turbulence above the telescope, which the most common ones is Differential Image Motion Monitor (DIMM). In optical testing, the Hartmann test is the common method to test the quality of optical components. ... Hartmann mask consists of 48 lenses. ...

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About us . ... Telescopes . ... Apart from the 6-meter telescope BTA two small telescopes are operative at SAO: the 1-m and 0.6-m telescopes, both manufactured by Carl Zeiss, Jena, are located near the BTA. ... These telescopes are used for adjusting the equipment and techniques of observations used at the BTA. ... The observational time allocation and also a brief description of the equipment of the 1-m telescope, which is used either permanently or mainly on this telescope, are presented below. ...

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• Lack of Dwarf Galaxies in the Local Volume Compared to Conventional Cosmology

... ДЖИНСЫ REGULAR ИЗ ТЕМНОГО ДЕНИМА СТРЕЙЧ-КОТОНА, С ДЕКОРАТИВНОЙ КОНТРАСТНОЙ СТРОЧКОЙ, ЗАСТЕГИВАЮТСЯ НА МЕТАЛЛИЧЕСКУЮ ПУГОВИЦУ И МОЛНИЮ. ... Цвет: синий . ... Радиотелефоны . ... Материал верха: искусственная кожа . ... Материал подошвы: полимер . ... Материал: искусственная кожа. ... Материал: ПВХ . Артикул - SB_SR-12,Бренд - Сибим (Россия),Коллекция - Среднерусская,Высота, мм - 1200,Материал - ПВХ,Цвет - зеленый . ... Цвет: зеленый . ... Цвет: экрю/серый меланжевый+коралловый/темно-синий . ...

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• Человек-паук 3 - Новый Диск / Beenox Studios - Новый Диск / Beenox Studios

... Gallery . ... Remains of dewars and small instruments fromтАж . Sidebar Left . ... Title: Remains of dewars and small instruments from the drawing office. Description: NOTE: All images and movies are copyright and must not be reproduced or mirrored in any form without written permission. ... Remains of dewars and small instruments from the drawing office. NOTE: All images and movies are copyright and must not be reproduced or mirrored in any form without written permission. ...

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• GSAOI Disk Galaxies Science Page
• Dougal Mackey - Research

... Science . ... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Properties of kinematically decoupled structures in Early-Type Galaxies . ... Science Users Information . ... ESO-MIDAS . ... ESO Science Newsletter . ... The project consists in measuring the stellar kinematics, stellar populations, dynamics, and morphological properties of the kinematically decoupled structures observed in the inner regions of Early-Type Galaxies. ... Return to list of thesis topics...

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• Sample Properties
• Properties of Young Massive Clusters | ESO
• Properties of Low-Mass Stars and Planets | ESO

... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...

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• Structure and properties of IRC+10216
• SMALL (МАЛЫЙ) - малый шрифт

... ICND-96, Saratov, Russia. ... And though a number of efficient methods of digital sound compression is developed by far, there is still a need in new efficient methods. In this report we study a possibility of application of fractal methods to compression of speech signals. ... In this method, a speech frame is divided into larger pieces called domains, and smaller ones called regions, and an optimal set of affine transformations of domains into regions is calculated. ...

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... Scientific goals . ... STUDY OF THE MARTIAN SURFACE COMPOSITION AND ITS PHYSICAL PROPERTIES . Main scientific objectives: . spectrophotometry of the planet in absorption bands of some rocks that may exist on the Martian surface in order to determine the surface composition; . study of the nature of aerosols by measuring spectral and angular distributions off brightness both above the planetary limb and of certain cloud-covered areas; . ... Main characteristics: . Spectral range . ...

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• DOK-2 Results Page
• Magnetic Fields
• MARSES Homepage | Instrument Information

... Natalya V. Raguzova and Sergei B. Popov . ... We present a compilative catalogue of Be/X-ray binaries and candidates in the Galaxy and in the Large and Small Magellanic Clouds. This catalogue contains 160 sources and provides information on names and spectral types of optical components, distances, on spin characteristics of neutron stars, and on orbital and X-ray properties of binary systems. ... Be/X-Ray Binaries and candidates in the Galaxy . Galactic sources: comments to the Table 1 . ...

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• Physicists on the Money
• The X-ray Optics
• PSR B0042-73 in the Small Magellanic Cloud

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• The Galaxy Gallery: Messier Objects
• Astronomy HyperText Book
• Orbital Properties of the Earth

Next: Copying Calibration Tables - Up: Calibration, the ATCA, and Previous: Determining Gains and Bandpass . ... This parameter can be used as an alternative way of specifying the XY phase of the antennas. ... Unless you explicitly turn off solving for XY phase in gpcal , then the only important XY phase value is that for the reference antenna. ... means that gpcal will solve for the XY phase of the reference antenna. ... By default it solves for all XY phases, except for the reference antenna. ...

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• Small_scope_radio_jove
• Basic Properties
• POLARIZATION PROPERTIES OF TWO PULSARS

Pulsar - the neutrone star. ... Its physical properties are greatly changed. ... Naturally after the discovery of pulsar connection with the remains of the supernew star outbursts it was supposed that the pulsars and the neutron stars are the same objects. ... In the external layer of a neutron star, where the substance dense is not so great to break the cores; they may from the hard chip structure, which at the pulsar rotation decreasing is broken the starquake. ...

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Next: Conclusions Up: HS 0822+3542 - a Previous: H I and dynamical . The properties of HS 0822+3542 presented above (extremely low abundance of heavy elements, very blue colour of underlying nebulosity, and extremely small mass ratio of stars to neutral gas) suggest that this could be the nearest candidate young dwarf galaxy forming its first stellar generation. ... Next: Conclusions Up: HS 0822+3542 - a Previous: H I and dynamical Labaratory "Structure" . ...

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• The statistical properties of HSS BCGs
• Instrument descriptors
• Signal detection

... Lets you work with numeric values. The Number object is an object wrapper for primitive numeric values. ... JavaScript 1.3: added toSource method . ... value . ... JavaScript 1.2: Number(x) now produces NaN rather than an error if x is a string that does not contain a well-formed numeric literal. ... The following example uses the Number object's properties to assign values to several numeric variables: biggestNum = Number.MAX_VALUE . ... ECMA-262 JavaScript prints the value Number.NaN as NaN . ...

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• A collection of images
• Objects, Methods, and Properties
• Virgo Group - Gravitational Wave basics

... 7.1 Introduction to media types . ... 7.3 Recognized media types . 7.3.1 Media groups One of the most important features of style sheets is that they specify how a document is to be presented on different media: on the screen, on paper, with a speech synthesizer, with a braille device, etc. Certain CSS properties are only designed for certain media (e.g., the 'cue-before' property for aural user agents). ... For example, the 'font-size' property is useful both for screen and print media. ...

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• Visual effects
• User interface
• Introduction to CSS2