... SMIS : Space Monitoring Information Support laboratory . Russia's Weather : State Meteorological Center Weather Forecast . Space Weather service : ACE real time solar wind data and simple geomagnetic activity forecast. ... World Fire Web : Space Research Institute (IKI) node . Sputnik : Joint project of SRC Planeta, Rosgidromet and Space Research Institute (IKI) . ... Today's Space Weather : Presented by the Space Environment Center . ... Back to the Space Research Institute Home Page ...

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• AZ Key parameters, 1997
• AZ Key parameters, 1998
• ENERGETIC PARTICLE EXPERIMENT DOK-2

The current set of keyword-value pairs of a task can be monitored by typing ESC K while the name of the task is present in the User Command Area. This causes (part of) the Common Output Area to be overlaid with a display containing the current user input parameters of the task. ... If there is currently a set of parameters displayed on the screen (as the result of typing ESC K ), these parameters will be edited; otherwise the name of the task is derived from the User Command Area contents. ...

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• User Parameters - Preparation of the Science field data CentralProcessor 0.11
• Central Processor Manager CentralProcessor 0.11 documentation
• SCINTILLATION PARAMETERS FOR 49 PULSARS

Observed maximum rotation velocity uncorrected for inclination effect. This quantity is calculated from 21-cm line widths at different levels and/or rotation curves (generally in H_alpha). ... These data are characterized by some secondary parameters: telescope, velocity resolution, level of the 21-cm line width and bibliographic reference. ... we start from a standard sample (a set of measurements giving a large and homogeneous sample). ... HyperLeda . ...

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• Documentation: LEDA: parameter: bar
• Documentation: LEDA: parameter:
• Mean astrophysical parameters from LEDA

. First page Back Continue Last page Summary Graphics .

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• The CIMA ALFA Instrument Monitor Window
• Index of /~phil/hardware/vertex/hagenDocmemos/klaus/ATA1A/parameter
• AGES Database Search

... Bayesian and maximum entropy algorithms that use a constant balancing parameter present large residuals in the low or the high S/N regions depending on the value chosen for the parameter. ... This variation of the balancing parameter implies a variable resolution in the restoration, allowing high resolution with low bias in high S/N regions and a lower resolution with lower artifacts in poor S/N regions. We have applied the algorithm to the FOC and WF/PC cameras of the HST. ...

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• N??ez LLacer: Image Restoration with Variable Resolution
• MIRI At A Glance
• Wavecal Parameters Table

Next: Other parameters of the Up: The Model Previous: Initial binary parameters . As we only deal with initially massive binary systems (their primary's mass is higher than 10 ), which are capable of evolving off the main sequence during less than years, the compact stars left behind stellar evolution are (in the case of the most massive stars) NSs and BHs. ... For a NS belonging to a binary, the evolution complicates as the secondary star evolves: for example, (recycling), etc. ...

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• Initial Distributions of Binary Parameters
• The Gravimagnetic Parameter
• The Effect of Relativistic Wind on Accretion Flow Parameters

XMM-Newton Science Analysis System . ... Meta Index / Home Page This section documents the parameters recognized by this task (if any). ... set . yes . ... frame exposuretimes below this value are flagged as bad (sec) . ... Add column with number of raw pixels per frame to EXPOSURE table . ... mark frames with more pixels above given level as bad . ... frames with more pixels than this level are flagged bad . ... 9999. 0. frames with a raw pixelrate above this level are flagged bad (pixels/sec) . ...

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AUTOMATIC STATION OF ECOLOGICAL CONTROL . ... BASIC PERFORMANCE SPECIFICATION . STATE OF ASEC DEVELOPMENT . AIR POLLUTION MONITORING . ... OF MEASURING CHANNELS . ... unit of measurement . ... Nitric oxide (NO) concentration, . ... power measured by ASEC . ... In particular, RSC Energia finalizes its work on measurement systems designed to measure dust, volumetric activity of radioactive gases and aerosols and other environmental parameters. ... Official WEB-site of S.P.Korolev RSC Energia . ...

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• INTERNATIONAL SPACE STATION

... Previous: Background Fluctuation Analysis from the Multiscale Entropy . ... A new measure of information is defined which is based on noise modeling and incorporates resolution scale. Properties of this measure are discussed. ... Additionally it allows for image noise modeling, and subsequent noise removal. ... Hence information- and entropy-based processing technologies will be necessary for the effective design and implementation of large, future generation, image databases. ...

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• Indexing and Searching Distributed Astronomical Data Archives
• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
• An Object Oriented Design for Monitoring the Chandra Science Instrument X-ray

... Other Characteristics of the Sun: Variability of Rotation, Magnetism, Chemical Structure, Planetary System. ... Methods of Solar Magnetic Fields Measuring: Visual, Photografic, Photoelectric. ... Empiric Datas of Magnetic Fields in Photosphere, Chromosphere and Corona. ... Characteristics of Magnetic Field in Balanced Force Tubes by Potential and Forceless Field. ... Phenomenons in Active Region (Magnetic Field, Spots, Torches, Solar Prominences, Flares, Discharges. ... Magnetic Fields in Flares. ...

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• ENERGOSPECTROMETER OF IONOSPHERIC PLASMA P3-3
• MISSION WARNING
• Optical static Fourier spectrometer

... 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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• Tutorial on Fortran 90, Digital UNIX

. Parameters of the Fabry-Perot Interferometers . Queensgate FPI . ICOS FPI . p260 . p501 . p751 . Order (in H-alpha line) . 235 . 501 . 751 . Interfringe (in H-alpha) . 28 A (1270 km/s) . 13 A (600 km/s) . 8.7 A (390 km/s) . Spectral range . 5000-7000 A . 5000-8000 A . 4500-9000 A . Finesse (in H-alpha) . 13 . 16 . 20 . Sp. resolution (in H-alpha) . 2.1A . 0.8A . 0.4A . Number of spectral channels . 24-32 . 36 . 40 .

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• On the problem of high spectral resolution observations of faint objects
• проект SCORPIO-2: parameters
• Optimization of spectroscopic observations

... SphereParams Struct Reference . ... SphereParams (const float radius) . ... Definition at line 50 of file StelGeometryBuilder.hpp . ... Definition at line 103 of file StelGeometryBuilder.hpp . ... Definition at line 120 of file StelGeometryBuilder.hpp . ... Definition at line 112 of file StelGeometryBuilder.hpp . ... Definition at line 118 of file StelGeometryBuilder.hpp . ... Definition at line 110 of file StelGeometryBuilder.hpp . ... Definition at line 114 of file StelGeometryBuilder.hpp . ...

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• Stellarium: RingParams Struct Reference
• Stellarium: TextParams Struct Reference
• Stellarium: StelGeometryBuilder Class Reference

... The project assumes creation of an international space observatory - the interferometer "Earth - Space - Space" in order to perform of astronomical investigations in millimeter, submillimeter and infrared regions with extremely high sensitivity (to a few nanoJanskies units of flux density in continuum spectrum) and extremely high angular resolution (to a parts of microsecond of arc or, possibly, nanosecond). ... radio-interferometric channels of the system "Space - Space", region 0.2 - 3 mm; . ...

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• Parameters of the Moon-perturbed orbit
• Description of the RadioAstron project, english version
• Results of measurements of SRT antenna parameters in Pushchino

... Guider functions . ... Guide Sensor Performance . ... Guide Sensor Sky Coverage/ Star Availability . Guide Star Selection Criteria . ... Guide fiber organization and reach at plug plate . ... Plug plate holes for guide stars are identical to those for science FO . ... FOV for each of 9 guide stars is 7.4 arcsec dia. (0.45 mm FO, Sumitomo IGN-05/10) . ... Selected guide stars must have no neighbor stars within TBD (5 arcsec) radius that have a brightness within TBD (5 mag.) of guide stars . ...

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• lsst.tcc: tcc.msg.formatObjFields Namespace Reference
• Telescope Parameters

The Ryle Telescope was used for some years for monitoring variable sources (in addition to its role in source-surveys related to the Sunyaev-Zeldovitch studies). The instrument is now transformed into the "AMI large array": see the AMI pages for details. ... The rebuild took place between 2006 June and mid-2008; between these dates there is no useful data available. ... For some sources there are many plots, organised by date: . ...

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• De-convolution of a Gaussian beam from planetary observations Bojan Nikolic web
• OptInt PmWiki : MROIDelayLineSW / Production Software FDR To Do List

makeprfcorr -- Compute the pixel response function for an image created with asncombine makeprfcorr association . association . ... Interactive program to compute relative shifts of images in an association file. ... After computing the relative shifts of the direct images, alignasn searches for corresponding grism images for each of the direct images. ... The grism association is then updated with the same relative shift measurements as determined from the direct images. ...

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• MAKEFLAT (Sep99) --- nictools --- MAKEFLAT (Sep99)
• ASNCOMBINE (Nov98) --- nictools --- ASNCOMBINE (Nov98)
• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)

To appear in "Fourth Workshop on Robotic Autonomous Observatories (2015)"RevMexAA(SC) MASSIVE PHOTOMETRY OF LOW-ALTITUDE ARTIFICIAL SATELLITES ON MINI-MEGATORTORA S. Karpov, 1, 3 E. Katkova,2 G. Beskin, 1, 3 A. Biryukov3,4 S. Bondar,2 E. Davydov5 E. Ivanov,2 A. Perkov,2 V. Sasyuk3 RESUMEN Favor de prop orcionar un resumen en espanol. ... The nine-channel Mini-MegaTORTORA (MMT-9) optical widefield monitoring system with high temporal resolution system is in operation since June 2014. ...

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• http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_meteors.pdf
• http://vo.astronet.ru/~karpov/pdf/2014_Sasyuk.pdf
• http://vo.astronet.ru/~karpov/pdf/2012_Searching.pdf

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Investigations of the ionospheric response to strong magnetics storms which are usual for our latitudes, are of great interest. ... In the figure, we present ionospheric parameter dynamics during three perturbed days in July 2000. ...

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• East Siberian Center for the Earth's Ionosphere Research. Specific character
• East Siberian Center of Earth Ionosphere Research. Chirp ionosonde.
• East Siberian Center for the Earth's Ionosphere Research. Modelling, secondary

... The variability of the spectrum of the optical component of the IR-source IRAS01005+7910 was discovered for the first time in the BTA spectra [1]. ... The spectral features include absorptions that form in near-photospheric layers, narrow envelope emissions, and emission-absorption profiles that form in photosphere-to-envelope transition layers (the wind). ... Discovery of spectral variation in the optical counterpart of IRAS01005+7910. ... Dashed line - envelope curve of all the SiII 5979 profiles ...

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• Solar system sector, archive 1993
• Hardware sector, archive 2004
• SAO RAS home page