... The reduction system of observations FADPS (description in Russian) (Flexible Astronomical Data Processing System) for data of wide-band receivers of the first observation cabin of the radio telescope RATAN-600 had been created under the Unix-like operational system DEMOS for computers of the SM-1420-type (PDP/11) in 1987 for observation analysis and estimates of coordinates and flux densities of radio sources. ... FADPS: flexible astronomical data processing system at RATAN-600 in UNIX environment....

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Disastrous earthquakes happen 100 to 200 times a year. ... There is a chance that the data of ionospheric plasma observations hold an answer to the latter question. Satellites and ground-based facilities may detect earthquake precursors in the ionosphere a few hours or days before the main shock. ... ULF "Hz"-oscillations have been recorded several hours before the main shock in a narrow magnetic field tube (40...100 km along the satellite trajectory) conjugated with epicenter of the earthquake. ...

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• Tomography
• Extragalactic Astronomy
• Mykola I. Dzubenko

On combined processing of different space geodetic observations . ... A software for combined processing of different space geodetic observations is developed along with the work on the co-location of various observational techniques at the observatories of Quasar VLBI network. ... Various aspects of the combined processing of different types of space geodetic observations are also discussed. ... space geodetic observations, combined processing, normal equations, software package, SINEX-format. ...

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• IAA EOP Service
• LAB Ephem. Astronomy-ERA
• (Untitled)

... A radio galaxy is a galaxy that emits an unusually big amount of energy at radio wavelengths. ... Inside of each galaxy with an active nucleus (radio galaxies are among them) there must be a system of a "central machine" responsible for the colossal amount of the emitted energy from radio to gamma ranges. ... Sometimes a radio source in an active galaxy may flare again if the needed conditions appear (a new portion of matter would fall into the furnace of the "central machine"). ...

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• Hardware sector, archive 2013
• Hardware sector, archive 2009
• The dust jets in the nucleus of comet 29P/Schwassmann-Wachmann 1

T he Siding Spring Survey (SSS) is a Near-Earth Object search program that utilises the 0.5-m Uppsala Schmidt Telescope at Siding Spring Observatory, N.S.W., Australia. ... The mission of the Siding Spring Survey is to contribute to the inventory of near-earth objects (NEOs), or more specifically, the potentially hazardous asteroids (PHAs) and comets (PHOs) that may pose a threat of impact and thus harm to civilization. ... Based on the CSS Mission page . ... Siding Spring Survey Main Page . ...

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• COALA - Computational Astrophysics Laboratory
• Mike Bessell, MSSSO - Images
• Marc White - Astrophysicist - The Australian National University

. The TV System for Navigation and Observation (TSNN) has been designed for solving navigation and scientific tasks of the "Phobos-Grunt" mission. Wide-angle . TV camera . TSNN includes four TV two narrow-angle and two wide-angle cameras. Every camera has built-in processor for real-time data processing. Each pair of TV cameras provides for stereoimaging. Narrow-angle . TV camera . Characteristics . Ground tests results . Publications

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• The Dynamo Process
• Gauss and the Global Magnetic Field
• The Sun's Magnetic Cycle

This composite image is based on observations from the New Horizons Ralph/LEISA instrument made at 6:25 a.m. EDT on July 14, 2015, when New Horizons was 50,000 miles (81,000 kilometers) from Charon. The spatial resolution is 3 miles (5km) per pixel. The LEISA data were downlinked October 1 4, 2015, and processed into a map of Charon s 2.2 micron ammonia-ice absorption band. ... The ammonia absorption map from LEISA is shown in green on the LORRI image. ...

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• Supernova simulations reveal new processes | Astronomy.com
• Processing your sketch | Astronomy.com

... Advises . Contact Advises . As an advise for amateurs we would like to underline: if it's possible, try to observe 3 asteroid positions per night and do not neglect to observe the Numbered Minor Planets in your telescope field of view as a "by product" of your observational programs. ... We think such estimations ought to be produced every morning after CCD observations of the moving celestial objects by observer himself. ...

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... Data processing and storage : · Processing time with Groningen cluster may exceed observation time , especially if thermal noise or high dynamic range or high resolution (international baselines) is requested · Other resources for data analysis should be investigated · Involvement of FZ JЭlich (1 PB storage and cluster processing ) is considered and will be tested, data transfer between Groningen and ...

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• Determination of the relative orientation between radio and dynamical reference
• G327.6+14.6
• PPEUC Programme - Cosmic Microwave Background Workshop

System of astrometric databases of Pulkovo observatory. 26-inch refractor . Pulkovo system of astrometric databases consists of three databases, which contain results of processing photographic and CCD observations, obtained with the 26-inch refractor and the Normal astrograph of Pulkovo observatory. Pulkovo photographic catalogs: Pul-2, Pul-3 (Pul-3 SE), Pul ERS . Results of photographic and CCD observations of Solar system objects . ... Normal Astrograph ...

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• Pulkovo databases: photometric observation

... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

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• Observing with VISTA
• Use of the (UK) VISTA Data Flow System
• VISTA - Visible and Infrared Survey Telescope for Astronomy

The problem of turbulence is one of the most important and challenging problem of the modern science. ... An experimental investigation of turbulent flows with special experimental setup and equipment, which allow to obtain reliable data with good precision, is very difficult and expensive process. ... The natural assumption for the theory of turbulence is that there exist some (unknown yet) general and universal properties for wide range of different turbulent flows. ...

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• The Sparkle Plug-In: Notes
• Adding new plug-ins to The Gimp
• APOD: 2010 June 20 - Abell 2218: A Galaxy Cluster Lens

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34. Follow Up - an Astronomy Net Observation_reports Forum Message

35. lsst.tcc: python/tcc/cmd/process.py Source File

36. http://www.astro.louisville.edu/shared_skies/archive/select/messier/m110/20121121/notes.txt

37. Fulbright scholar Leonid Zotov

38. PLANETA home page

39. ApSA courses

40. Conference "Random Processes, Conformal Field Theory and Integrable Systems"