... Data was taken with lbw and the mock spectrometers on 05may09 to investigate the problem with higher time resolution and bandwidth. ... 6 172 Mhz bands were taken centered at: 1200,1300,1400,1500,1600, and 1700 Mhz. 8192 channels (20Khz resolution) was used for the low time resolution (.1 second dumps). 4096 channels (40Khz resolution) was used for the high time resolution (.001 second dumps). ... The total power was computed for each 172 Mhz band and then plotted vs time (.1 second resolution). ...

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• punta salinas,alfa 02nov11
• aerostat returns apr14
• high resolution decimation test

... HST . ... Data . ... HST Overview . Overview . ... Instruments . ... Instrument Handbook . COS Data Handbook . ... For more information about the use of this FP-POS option see Section 5.8.2 of the COS Instrument Handbook. ... COS has the advantage of a fairly large aperture so that there are only small aperture losses ( see Section 5.1.9 of the COS IHB). ... The available spectroscopic resolving powers (R) available to observers with COS are listed in Table 5.1 of the COS Instrument Handbook. ...

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• COS Data Handbook
• ACS Instrument Handbook for Cycle 20
• Space Telescope Imaging Spectrograph Instrument Handbook

... We can help students grasp the significance of Hubble's extremely keen eye, and learn a bit about angles and math in the process, with the following in-class activity. ... Looking through binoculars or telescopes allows us to magnify a small section of the sky. To measure sizes or distances in that small section, astronomers divide a degree into 60 smaller pieces called arcminutes, and further subdivide minutes into 60 smaller sections called arcseconds. ... 30 feet = . ... 36 seconds . ...

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... ATNF Home . About ATNF . ... About ATNF overview . ... Governance overview . Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Our people overview . ... Publications overview . ... ATNF facilities . ... Parkes radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... Images . ... The MAPPIT (Masked APerture Plane Interference Telescope) instrument has been used for NRM observations at the 3.9m Anglo-Australian Telescope. ...

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• Australia Telescope Compact Array Home Page
• difx:ivs2016extras [ATNF VLBI Wiki]

... Lightning Captured at 7207 Images per Second . ... 23.07.2012 . ... Credit Copyright: Tom A. Warner , ZTResearch , www.weathervideoHD.TV Explanation: How fast is lightning? ... The above lightning stroke did not move too fast, however, for this extremely high time resolution video to resolve. Tracking at an incredible 7,207 frames per second, actual time can be seen progressing at the video bottom. ... July 2012 . ... 2011 2012 . ... NASA Web Site Statements, Warnings, and Disclaimers . ...

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• Journal "Peremennye Zvezdy"
• Астронет > Lightning Captured at 7207 Images per Second
• XWare > APOD

... Science . ... Science Users Information > Science and Technical Meetings > Conferences 2012 > Circumstellar Dynamics at High Resolution . ... Observing with ESO Telescopes . ... Data Handling and Products . ... If you are interested in participate in the workshop please fill out the registration form . ... The workshop will take place in Foz do Iguaцїu, Brazil, close to the magnificent Iguaцїu Waterfalls, a network of 275 waterfalls in the Iguaцїu River that lies in the border of Brazil and...

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• CRIRES - VLT High-Resolution IR Echelle Spectrometer
• ESO - Galaxies2015
• ESO - VLT/Instrument Interfaces

. Next: To both compress and Up: *display, xdisplay, xexamine* - Previous: *xdisplay* - Image Display . Display just the section of interest: . tv> xdisplay ``xdata$rp110590.qp[6700:7200,9100:9600]'' # range of x coord is 6700-7200, # range of y coord is 9100-9600. rsdc@cfa.harvard.edu . 1998-06-10

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• Source Selection
• Spatial Region Coordinates
• Everyday Classroom Tools: Table of Contents

... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2012 July 23 . Lightning Captured at 7,207 Images per Second . ... Explanation: How fast is lightning? Lightning , in fact, moves not only too fast for humans to see, but so fast that humans can't even tell which direction it is moving. ... Follow APOD on: Facebook ( Daily ) ( Sky ) ( Spanish ) or Google Plus ( Daily ) ( River ) . ...

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• Pulse-per-second (PPS) Signal Interfacing
• APOD: 2005 July 5 - Thirteen Seconds After Impact
• APOD: July 30, 1999 - The Sea of Tranquillity: 5 Seconds To Impact

... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...

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• Evidences of supercritical accretion onto black hole in SS433
• Solar system sector, archive 2011
• Hardware sector, archive 2009

... First of all, I should say that you cannot guarantee user-mode processes to have exact control of timing because of the multi-tasking nature of Linux. ... However, for most applications using I/O ports, this does not really matter. To minimise this, you may want to nice your process to a high-priority value (see the nice(2) manual page) or use real-time scheduling (see below). ... Linux 2.x kernels have soft real time support; see the manual page for sched_setscheduler(2) for details. ...

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• The prime focus echelle spectrograph and the MSS
• Results scientific researchs 18
• High resolution Zeeman spectrum of HD4778

... The three optical trains for the cameras, and the pupil reimaging system, are mounted on a wheel, accurately driven by an external motor. ... The low-resolution spectroscopic mode uses the wide field camera and a suitable set of grisms and order sorting filters that are inserted in the parallel beam after the pupil. ... One of the five grisms can operate at four different orders, depending on the filter selected on the first filter wheel that acts as order sorter. ...

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• Ranger 7
• Ranger 9
• Ranger 8

... The greater the distance, the smaller the parallax. ... That triangle has the same proportions as the much larger triangle ABC, and therefore, if the distance B'C to the thumb is 10 times the distance A'B' between the eyes, the distance AC to the far landmark is also 10 times the distance AB. ... The most distant objects our eyes can see are the stars, and they are very far indeed: light which moves at 300,000 kilometers (186,000 miles) per second, would take years, often many years, to reach them. ...

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• Newton's Second Law
• ENERGETIC PARTICLE EXPERIMENT DOK-2
• Trigonometry beyond 90 degrees

... SkalnatЄ Pleso 43, 1 ґ 2, (2014) e Mini-MegaTORTORA ґ 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/2015_Terskol_mmt_meteors.pdf
• http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_meteors.pdf
• http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt.pdf

... 2MASS Overview . The 2MASS Sky . Executive Summary of 2MASS Second Incremental Data Products . Point Source Catalog . Extended Source Catalog . ... Distribution Mode for 2MASS Products . Data Release Plan . ... Point Source Catalog (PSC) . Extended Source Catalog (XSC) . ... 2MASS Source Naming Convention . ... General Properties of the Data Release . ... Comparison of Achieved Performance of Second Incremental Release Catalogs with Level 1 Science Specification . ...

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• Order Definition
• New CCD detector for macromolecular diffraction data
• Selection of ELG candidates from objective prism spectra

... Kepler's Laws . ... Second Law . 12a. More on 2nd Law . ... Kepler's 2nd law prescribes the way the velocity V of an object orbiting a single center varies around its orbit: . The rate at which the line to the center ("radius vector") covers area does not change around the orbit." As noted in section #12 , this means that the object's velocity V increases when its distance r decreases, and vice versa. ... Because by Kepler's 2nd law, the Earth moves in its orbit a little faster in winter. ...

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• Newton's Second Law
• Folding Paper Model of Magnetosphere
• HYPERBOLOID Results Page

... Average resolution at altitude H=668 km . ... Swath width at H=668 km and inclination of beginning of swath 20.48 degrees . ... Resolution at H=668 км . ... Наименование параметра . ... 1 канале . ... Полоса обзора при H=668 км . ... 1-5 спектральной зоне, не более . ... 1 спектральной зоне . 0,48-0,52 мкм . ... 0,915-0,997 мкм . ... 1-4 канал . ... 1-4 каналов . ... Спектральные характеристики каналов (по уровню 0,5): . ... For more information send a mail to: info@sputnik.infospace.ru . ...

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Static Fourier spectrometers are often used for spectral measurements of the ionosphere emissions. There are two main advantages of Fourier spectrometers (FS) - large geometric factor and high spectral resolution; these parameters are two orders better than for grating spectral instruments. ... In scanning Fourier spectrometer optical and electric modulation of signal is used to avoid this problem, for static Fourier spectrometer there are no such ways. ...

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• ENERGOSPECTROMETER OF IONOSPHERIC PLASMA P3-3
• Explanation of the table of ecliptical coordinates of the Sun.
• MISSION WARNING: The Second International Meeting : Protocol

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Time series at time resolution of 4 seconds and 17 minutes are shown in red and blue respectively, with RMS noise of 65 mJy for the 4 second resolution time series and 4 mJy for the 17 minute resolution time series. No evidence for heightened emission is present during any of the observed orbital/rotational phase of the planet. ... Last Revised: 2012 October 31st . ...

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• Explosive Events
• Armagh Observatory Weather in July
• Follow up from the Second Cross-Border Schools Science Conference |

... 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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• Image: In the bus, on the second floor
• Image: Dragon on the rooftop (view from the restaurant at the second floor).
• Long description for the second Bach/XML formatting example

... NIC-FPS is an instrument combining the capabilities of a near-infrared imaging camera with a cryogenic Fabry-Perot etalon currently under development at the Center for Space Astrophysics and Space Astronomy , University of Colorado with support from Rice University , Ball Aerospace and the Astrophysical Research Consortium. It is scheduled to begin operations on the ARC 3.5m telescope at Apache Point Observatory in 2004. ... For full frame images, the FITS file will result in a size of: . ...

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• Spectrographic time budget
• Manastash Ridge Observatory Directions Page
• Tilt and Sag Coefficients: 14 Apr 2000