adapted from Observe: Eclipses, published in 1979 by the Astronomical League and "Safe Solar Filters," by B. Ralph Chou, Sky and Telescope, August 1981) . ... Tape TWO pieces of film together into a sandwich, and tape this over the opening in the cardboard. ... The cardboard frame will act as a shade from the bright Sun, while you safely observe through the film sandwich. ... Undeveloped film is not safe. ... tape . ... At the end of one of the tubes, tape the aluminum foil, and make a tiny pinhole. ...

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• ASP: Making a Rainbow
• ASP: Beacons in the Gloom

... Next: Star Finding and Up: Image Restoration and Previous: Multiresolution and Astronomical . ... Design improvements continue to be made in the filter developed using mathematical morphology principles for the Infrared Astronomical Satellite ( IRAS ) images. The purpose of this filter is to eliminate Galactic cirrus emission from extragalactic fields. ... With an appropriate normalization, the filter curve was applied to each pixel in the image to remove the Galactic cirrus. ...

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• A New Entropy Measure Based on Multiple Resolution and Noise Modeling
• Noise Detection and Filtering using Multiresolution Transform Methods
• Application of a Kalman Filter at UKIRT

... Data Reduction FAQ > A number of OmegaCAM filters show vignetting in their central regions. What are the causes for this and what are the dimensions of these features? ... Observing with ESO Telescopes . ... ESO-MIDAS . ... ESO Data . ... ESO HST Image Galleries . ... ESO Data Access Policy . ... ESO Science Newsletter . ... A number of OmegaCAM filters are not monolithic, but consist of four segments (each covering 8 detectors) that have a central cross-shaped support structure. ... Filter . ...

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• Images of SCR 1845-6357 A and B in different filters (NACO-SDI/VLT)
• State-of-the-art digital filter circuit boards for the ALMA correlator
• Limb darkening

. unfiltered . GGM02C model . PC 1 . PC 2+3 . PC 2 . PC 3 . PC 4 . PC 5 . Sum of nine first PCs 2-10 . Difference between the initial signal and ten first PCs 1-10 . PC 1 . PC 2+3 . PC 2 . PC 3 . PC 4 . PC 5 . Sum of nine first PCs 2-10 . Difference between the initial signal and ten first PCs 1-10 . PC 1 . PC 2+3 . PC 2 . PC 3 . PC 4 . PC 5 . Sum of nine first PCs 2-10 . Difference between the initial signal and ten first PCs 1-10 .

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• Fulbright scholar Leonid Zotov
• Leonid Zotov

... Tonight's Sky . ... Observing . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Filtered solar views . ... With the range of filters and telescopes available for solar observing these days, we have never had a better opportunity to safely observe the Sun from the comfort of our backyards. ... Get instant access to subscriber content on Astronomy.com! ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...

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• How do light pollution filters work? Do they actually help? | Astronomy.com
• Maximize a minimum filter | Astronomy.com
• filter | Astronomy.com

... LUMAM . ... HOME . ... ABOUT LOMO . ... MICROSCOPES . ... SURGICAL MICROSCOPES . ... Home Products Microscopes Lumam Fluorescence filters . LUMAM FILTER CUBES . Filter Cube Sets from OMEGA® Optical, Inc. ... 575.00 . ... Filter Cube Sets from LOMO® . ... 395.00 . ... LOMO America, Inc. ... 2000-2016 LOMO America,Inc. ...

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... Segmentation of the solar radioimages . ... To find out faint contrast formations in distributions of radiobrightness of the solar corona, received at wavelength 5.2 sm on the Siberian solar radio telescope (SSRT), we develop algorithm on the basis of updating the Wiener-Tikhonov's filter with operated parameters and the high-frequency contrasting filter. ... The corresponding software is developed for processing radioimages of the Sun by this method of recognition of faint contrast formations. ...

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• Keywords_506
• Keywords_96

RTT150 . Russian-Turkish 1.5-m Telescope . ... Until 2002 observations were mostly performed with ST-8E CCD in the 1:7.7 Cassegrain focus. ... In April, 2003 telescope was equipped with a larger-size CCD Andor DW436 . ... 2048 x 2048 pixels, . ... Since summer of 2002 the main focal detector of the RTT150 telescope was AP47p CCD in 1:7.7 Cassegrain focus. ... During September 3-13, 2002 works on installation of new autoguiding system ( photo 1 ) were carried out on RTT150 telescope. ...

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• Test images from RTT150
• Russian Turkish 1.5-m telescope
• Программа наблюдений на RTT150

vlf.tab . vlf.txt . 00123a3a.dat 00136a3a.dat 00305a3a.dat 00371a3a.dat 00384a3a.dat 00463a3a.dat 00490a3a.dat 00581a3a.dat 00642a3a.dat 00647a3a.dat 00655a3a.dat 00668a3a.dat 00671a3a.dat ...

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• GRB observations
• Laboratory facilities for science education and research
• The magnetometer SG-R8

... Речь идет о программе обработки фотометрических наблюдений. К сожалению, пока программа работает только в MS DOS! ... используя специальные наблюдения стандартных звезд, и . используя наблюдения звезд сравнения (при определенных условиях); . ... Комплект включает в себя руководство по использованию в форматах LaTeX и DVI, примеры входных файлов данных и исполняемый файл. ... Обязательно нажмите клавишу SHIFT перед тем, как щелкнуть мышкой по merl.exe . ...

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Stellarium 0.12.3 . ... FileљStructure . ... TextureParams Struct Reference . Parameters specifying how to construct a texture. More... #include < StelTextureParams.hpp > . ... filtering (const TextureFiltering filtering) . Set texture filtering mode. ... Texture filtering mode. ... Default parameters (no mipmaps, linear filtering, clamp to edge wrap mode). ... TextureParams c = TextureParams ().generateMipmaps() .filtering(TextureFiltering_Nearest).wrap(TextureWrap_Repeat); . ... wrap . ...

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• Stellarium: ShortcutsFilterModel Class Reference
• Stellarium: SatellitesListFilterModel Class Reference
• Stellarium: Member List

... The filter "Lighting Effects" is a freebie that came with this program, and in my opinion is practically worth the whole purchase price all by itself. ... You can select different light sources, and combine them with texture channels to warp your image. ... Depending on how you use it, pure white is the highest point on the image, and black the lowest. ... You can adjust the brightness and spread here, or choose other types of lighting. ... Use these if your image is turning out too dark or light. ...

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• Hands On; The Button Mask
• Torsten Martinsen's GIMP plug-ins
• GIMP: Tips and Tricks for Creating Images

A computer controlled low light photometer for nightglow observations. Hardware units of portable photometer for low light measurements, especially night glow emission is described. ... Interface card contain three channels of 24 bit counter, 4 channels of 12 bit ADC and the buffer bus for the controlled motors of the altazimuthal fork mounting and filters wheel, the position encoders. ... Where N( ) is output signal photometer generated input light flux F( l ) . ... PMT # . 599 . ...

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.

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• rtftohtml Users Guide - 2 How it works
• rtftohtml Users Guide - Title
• rtftohtml Users Guide - 3 What about Graphics?

The 25th International Symposium on Space Terahertz Technology , 27 ­ 30 April 2014, Moscow, Russia Capillary quasioptical highpass filter Valerian S. Edelman , Mikhail A. Tarasov and Artem M. Chekushkin . ... Matrix of capillaries can operate as a high pass filter at millimeter and submillimeter waves without additional adapters. ... For inner diameter of capillary of 0.7 mm and length of 3 mm the attenuation of such filter was over 40 dB at frequencies below 200 GHz. ...

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• http://www.cplire.ru/html/lab234/pubs/2012_13.pdf
• http://www.cplire.ru/html/lab234/Tarasov/reprints/PhysicaC2002p171.pdf
• http://www.cplire.ru/html/lab234/pubs/2009-06b.pdf

Lab . Main page News People . ASA . Master . Master net Homepage . ... Lomonosov Moscow State University Sternberg Astronomical Institute . ... MASTER . ... Lomonosov (ShOK) . ... About Space Monitoring Laboratory, scientific directions, instruments, contacts . People, who work in lab . Latest news and news archive . ... GRB 100131A: MASTER-Amur alert observations 76 sec after Notice time.The limit of the main telescope images is aboute 15 mag (unfiltered). ... All news ...

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• Общемосковский семинар астрофизиков имени Якова Борисовича Зельдовича

AMPLITUDE AND PHASE VARIATIONS OF THE CHANDLER WOBBLE FROM 164-YR POLAR MOTION SERIES Z.M. MALKIN, N.O.MILLER Central Astronomical Observatory at Pulkovo of RAS Pulkovskoe Ch. ... The CW amplitude and phase variations were examined by means of several methods which yield very similar results. ... To extract the CW amplitude and phase variations from the filtered PM series two different techniques were used. ... The CW amplitude variations are shown in Fig. 1 for two methods used. ...

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• ASTROMETRIA
• Magnetic fields database
• Selection from the database

Системные исследования и разработка спутниковых систем ДЗЗ; . Разработка и создание бортовых радиометрических средств в СВЧ-диапазоне; . Разработка методов дистанционной диагностики процессов в системе океан-атмосфера с помощью спутниковых средств СВЧ-радиометрии (синоптические океанические вихри, фронтальные зоны, течения, волны Россби, тайфуны и ураганы, явление Эль-Ниньо). ... Директор . ... 1-ый заместитель директора . ... 2014 НТЦ "КОСМОНИТ" ОАО "Российские космические системы" . ...

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K. Baur ETH Zurich Zurich, Switzerland karin.baur@math.ethz.ch -filtered mo dules for a self-injective Nakayama algebra We describe the class of -filtered modules without self-extension for the Auslander algebra of a certain self-injective Nakayama algebra. The motivation for this is to model the P -orbits in the nilradical of a parabolic subalgebra p = LieP where P is a parabolic subgroup of an even special orthogonal group. This generalises work of Bruestle, Hille, Ringel and Roehrle (1999). ...

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• Basic set theory (Spring 2003)

MASTER OT J035815.59+214117.9 discovery - dwarf nova outburst MASTER-Kislovodsk auto-detection system discovered OT source at (RA, Dec) = 03h 58m 15.59s +21d 41m 17.9s on 2015-11-18.89742 UT. The OT unfiltered magnitude is 17.1m (limit 18.1m). The OT is seen in 3 images. There is no minor planet at this place. We have reference image without OT on 2010-12-03.85624 UT with unfiltered magnitude limit 20.2m. Spectral observations are required.

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• http://observ.pereplet.ru/MASTEROTJ115059.36-342142.2.html
• Обсерватория