... Skalnatґ Pleso 43, 1 ­ 2, (2014) e Mini-MegaTORTORA ­ multichannel system for wide-field optical monitoring with high temp oral resolution V. Sasyuk1 , G. Beskin2 , S. Karp ov2 , S. Bondar3 , A. Perkov3 , E. Ivanov3 , E. Katkova3 and A. Shearer4 2 Kazan Federal University, Russia Special Astrophysical Observatory of Russian Academy of Sciences, Russia 3 Insttitute for Precise Instrumentation, Russia 4 National University of Ireland, Galway, Ireland Received: November 4, 2013; Accepted: ?? ...

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• http://vo.astronet.ru/~karpov/pdf/2013_EAS_Karpov.pdf
• http://vo.astronet.ru/~karpov/pdf/2015_Terskol_mmt_meteors.pdf
• http://vo.astronet.ru/~karpov/pdf/2012_Searching.pdf

... European Remote Sensing Satellite (ERS-1) was launched on 17 July 1991, and the follow mission ERS-2 (with the same sensors and an Ozone monitoring instrument added) was launched on 21 April 1995. ... ERS-2 has a fixed repeat cycle of 35 days, and follows ERS-1 tracks with one day's delay. ... Swath width is 102.5 km (telemetered), spatial resolution is about 25x25 m. The Advanced SAR (ASAR) instrument is carried by ESA's ENVISAT satellite launched on 1 March 2002. ... Swath . ... Spatial Resolution...

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• Environment Monitoring Information Systems
• Polar Orbiting Satellites
• ENERGETIC PARTICLE EXPERIMENT DOK-2

... 06jun11: testing the compressor monitor system on the telescope. 14apr11: testing the compressor monitor system in the lab . ... Around second 400 to 500 seconds, willie iguina openned the huffman box of the compressor monitor to get access to turn off the device. ... luis added some shielding to the devices in the huffman box (.pdf) and then remeasured the rfi on 15apr11. data was only measured up to 2500 MHz on this data with the huffman box closed. 902 probe: rfi below 100 MHz way down . ...

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• Galactic ALFA Surveys
• sitePwrshutdown 1999
• high resolution decimation test

To main of Laboratory . The research work and design of optical and optical-electronic devices are carries out by laboratory staff: . ... Lens: . ... In the layout 1 prism systems perform functions of dispersive element, corrector of aberrations, optical reducer. ... Spectral range 200 - 400 nm; . ... Back Forward . ... The main corrector's function are compensation of field aberrations of the main spherical mirror of a telescope (diameter of 600 mm, f'=1200 mm) and increase aperture ratio. ...

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HUBBLE SPACE TELESCOPE DAILY REPORT #1002 PERIOD COVERED: 0800 EST Daily Status Report as of 300/1200Z. 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed GHRS/2 5041 (GHRS Sensitivity Monitor - Cycle 3) The High Resolution Spectrograph was used to make 24 ultraviolet observations of standard star AGK81D266 to monitor the sensitivity of the HRS, which is expected to change slowly with time. ... Cycle 3 High) 3.7 Complete WFC 5076 (WF/PC Cycle 3 Calibration: WFC Flats Wide. ...

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• http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_01_14_94
• http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_09_14_95
• http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_04_21_94

Swift/ XRT radiation damage and results from the lab using a proton-damaged CCD Claudio Pagani (Swift/ XRT team) XMM Calibration Meeting, Leicester, 7/3/2012 XRT CCD e2v CCD -22 detector (developed for EPIC MOS camera on XMM) Operated in Photon Counting (PC) and Windowed Timing (WT) mode 4 55Fe corner sources continuously illuminate CCD corners, used to monitor CCD performance Spectral resolution at launch: FWHM = 135 eV at Mn K- (5.9 ...

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• Generation from In-Orbit Data
• XMM-Newton Radiation Monitor Details

... The remote planet Pluto and its moon Charon orbit the Sun at a mean distance of almost 6,000 million kilometres, or nearly fourty times farther out than the Earth. During a recent investigation by an international group of astronomers [1], the best picture ever of Pluto and Charon [2] was secured with the European Space Agency's Faint Object Camera at the Hubble Space Telescope (HST). ... The new HST image was taken when Charon was near its maximum elongation from Pluto (0.9 arcseconds). ...

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• ESO - High Resolution 2014
• ESO - HIRES 2014: Astronomy at High Angular Resolution - A Cross-disciplinary
• ESO - Why do the flats in my data have different exposure times and how do I

Next: Extraction of Information Up: Image Manipulations Previous: Transformations . ... Basically, it is not possible to retrieve information on features with frequencies higher than the Nyquist frequency (see Equation ). Several different techniques are used depending on the data (see Wells 1980 for a general discussion of the methods). ... Another group of image restoration algorithms use iterative methods to obtain a solution which is consistent with the data. ...

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• HyperLEDA: documentation
• HyperLEDA Internal documentation
• Optical spectroscopy

... RADIATION AND ECOLOGICAL MONITORING . ... OF MEASURING CHANNELS . Parameters of ecological fields measured by ARES . Parameter measured, . ... Volumetric activity of gases radionuclides in the air, Bq/m 3 : . ... of inert gases . ... Volumetric activity of a- and b-active aerosols, Bq/m 3 : . ... Concentration of nitric oxide NO, mg/m 3 . ... Meteorological parameters measured by ARES . ... 0.5 + 0.05 V), where V - measured wind velocity . ... Official WEB-site of S.P.Korolev RSC Energia . ...

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... 2011 February 7 . Sun 360: STEREO Captures Views of the Entire Sun . Credit: STEREO Project , NASA . ... This has become possible because the two STEREO satellites orbiting and monitoring the Sun are now on opposite sides of the Sun. ... Even though the STEREO satellites will continue to drift apart at about 44 degrees per year, Sun-staring instruments on or near the Earth will augment them to provide a full view of the Sun for the next several years. ... About APOD | ...

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• APOD: 2005 October 5 - An Annular Solar Eclipse at High Resolution
• APOD: 2002 October 24 - Gullies on Mars
• APOD: 2006 August 2 - Methane Rain Possible on Titan

... The value of tile-size, NW , may be thought of as a sixth coordinate axis in the chirplet transform parameter space - TF-area. Including this sixth coordinate axis provides us with a hierarchical (multi-resolution) CCT. ... Various 2- D slices through the multiresolution CCT may correspond to useful tilings of the TF plane with true parallelograms (true to the extent that the DPSS define a truly rectangular region in the TF plane). ...

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• Warp Fix - S3 with GENDAC enhanced BIOS
• Long description for the illustration of reference vs. device pixel
• Photo album: Japan: Kyoto and Nara, August 1997

Next: Rotation Periods of ZAMS stars Previous: T Tauri Stars . ... The first attempts to directly measure periodic modulation of T Tauri stars occurred in the early 1980s. Rydgren & Vrba (1983) observed four PMS stars using photoelectric photometry over a period of seven consecutive photometric nights. ... Because the spot lifetime is much longer than the rotational period, the observed effect will be a modulation of the light from the star synchronously with the rotation period. ...

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• Source Selection
• Microcalorimeters
• The Orion OB1 Association

... In combining the data, it is assumed that the low resolution image better represents the short spacing data, whereas the high resolution best represents the fine structure. ... Key: out The output image. ... Key: factor The flux calibration factor. ... In practise, the calibration may not be perfect, and an extra calibration factor will be required to align the flux scales. "factor" gives the factor to scale the low resolution image to put it on the same flux scale as the high resolution image. ...

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• Bandpass and antenna gain calibration
• Weighting
• casacore: casa/BasicMath/Functors.h File Reference

... In January 2015 using the Mini-MegaTORTORA multichannel optical sky-monitoring system with subsecond temporal resolution, the observations of comet C/2014 Q2 (Lovejoy) and asteroid 357439 2004 BL86 were carried out. ... It was put into operation in 2014. ... Comet C/2014 Q2 (Lovejoy). The 60-min-long observations with the Mini-MegaTORTORA system on Jan 19, 2015 at 16:50 UT, exposure time 30 s, BVR synchronously . ... Asteroid 357439 2004 BL86. ...

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• SAO RAS home page
• IRAS01005+7910
• Hardware sector, archive 2014

... Let us first find out which way -- rise in spectral resolution with some loss in the S/N ratio or increase in the S/N ratio with a fixed spectral resolution -- is better for the purpose of reduction of equivalent width determination errors. ... N -- number of counts for 1 ? ... line equivalent width, . ... Thus if the spectral resolution is managed to be increased (i.e. to decrease )without loss in the number of counts falling at 1 ?, the equivalent width measurement error is then proportional to . ...

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• Instrumentation
• Results scientific researchs 18
• On the problem of high spectral resolution observations of faint objects

Solar High Resolution Studies . ... Solar Group . ... High Resolution Studies . Small Scale Activity . ... High resolution observations at different heights in the solar atmosphere have emphasized that there is no such thing as a "quiet" Sun (e.g. Schrijver et al., ... This, and the temporal coincidence of other signatures, supports the idea that microflares are indeed just miniature flares, but that one needs a very high resolution in order to observe them (Cauzzi et al., 2003, in preparation) . ...

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• Observing capabilities
• The Face on Mars
• High-resolution Herschel spectroscopy reveals the proto-planetary disk around

... CYGAM FLIGHT IN THE HIGH APOGEE ORBIT? Distribution of the Galaxy diffuse emission with high angular resolution allowing to refine the spatial distribution of the cosmic-ray protons in the Galaxy. More than 1000 compact sources with the fraction of degree location accuracy and continuouse monitoring of their flux time variation. Up to 10 new gamma-ray pulsars emitting in the very high energy range. Several high energy gamma-ray bursts with the fraction of degree localization accuracy. ...

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• Spacecraft Digital Imaging Cameras
• Main research and development work completed in 2012 and ready for
• Polar Orbiting Satellites

WPLTN Technical Workshop . ... WPLTN-2012) . ... of the International Scientific Technical Conference WPLTN-2012 . ... Having an opinion that the collocation of various space geodesy measurement technologies has a fundamental role in increasing the accuracy of fundamental and applied positioning, navigation and timing provision, the International Scientific Technical Conference WPLTN-2012 has come to the following conclusions: 2.1. ... Web-page . ... Resolution of the conference WPLTN-2012 . ...

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• (Untitled)

... Detector - Machine Data Flow · Detector - Machine diagnostic info (slow) · Detector - Machine feedback inputs (fast) · Machine - Detector information Eric Torrence 2/8 July 2004 Polarimeter 532 nm Frequency Doubled YAG Laser e­ Mirror Box Pockels Cell Left or Right Circularly Polarized Photons Focusing and ... Eric Torrence 7/8 July 2004 Putting it all together Beam Instrumentation historically runs in a semi-autonomous manner from either machine or detector. ...

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• http://zebu.uoregon.edu/~uochep/talks/talks06/vlcws-sinev.pdf
• http://zebu.uoregon.edu/~uochep/talks/talks04/beam11-04.pdf
• http://zebu.uoregon.edu/~uochep/talks/talks02/G020349.pdf

This directory contains Calgary Neutron Monitor Data at five minute resolution. Each file is a gzipped tar archive that contains files of uncorrected count rates and barometric pressures at five minute intervals for one year. A file named snm.calg.fmi.YYYY.tgz is an archive that holds five minute data for the year YYYY. ... So a file named cal01030.fmi contains five minute uncorrected data for year 2001 day 30 (which is Jan 30, 2001). ... A text file named note.txt is also usually present. ...

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• http://www.wdcb.ru/stp/data/cosmic.ray/G%20L%20E/C065/GLE%2365.TXT
• http://www.wdcb.ru/stp/data/cosmic.ray/G%20L%20E/C066/GLE%2366.TXT