... 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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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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• Central Processor Manager CentralProcessor 0.11 documentation
• Duchamp Source Finder
• FlagTask CentralProcessor 0.11 documentation

... Source definition list: a dataset containing the SRCLIST table, and to which the region extensions will be added. evlist . ... The dispersion-axis spacing of vertices for image regions and the spatial background region, specified as the number of vertices across a node. ... Downward size of image regions, specified by the percentage of the cross-dispersion PSF covered between the source cross-dispersion off-axis angle and the lower of each pair of vertices with the same dispersion coordinate. ...

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Beam Instrumentation Overview November 14th, 2004 WG4 - Beam Delivery/Interaction Region First ILC Workshop KEK Eric Torrence University of Oregon З Largely personal viewpoint З Re-written to remove head-on references Eric Torrence 1/15 November 2004 Topics Beamline Laserwire BSL Monitor Polarimeter Spectrometer Diagnostic Physics Pair Monitor Bunch Length Detector Veto Bhabha Acol Wide variety of topics Very broad overview.. ... Eric Torrence 12/15 November 2004 Collision Biases in s - 2 E b vs. ...

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• http://zebu.uoregon.edu/~uochep/talks/talks05/torrence_mdi.pdf
• http://zebu.uoregon.edu/~uochep/talks/talks05/srtor01-05.pdf
• http://zebu.uoregon.edu/~uochep/talks/talks05/torrence_eintro.pdf

... QC1 database . ... The quality information is derived in form of QC1 parameters. ... The Health Check monitor collects QC1 parameters and their scores. ... The results are presented in two views: the graphical HEALTH CHECK monitor with the full trending reports, and the QUICK-LOOK monitor with scores. ... The Health Check Monitor is a joint effort of the Quality Control Group in Garching and of Paranal Science Operations. ... You can download the QC1 parameters, and also connect to the QC1 database....

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• Health Check Monitor: Users Guide
• Preparation of parameter file
• Score report for UVES.2012-01-29T09:00:11.500_tpl.ab

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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... Figure: Massive binary evolutionary track. ... A short glance to this track is sufficient to understand that there are a lot of evolutionary scenario parameters, which affect different stages of the binary evolution. Fortunately, a very limited number of parameters has effect on the compact binary merging rate. ... The most important (and practically unique) parameter changing the galactic binary NS merging rate is the distribution of an additional (kick) velocity imparted to NS at birth. ...

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• No Title
• Dependence on the Scenario Parameters and Initial Distributions
• Contents

... 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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• TUI:Scripts:Scripting Tutorial:Loops

... This section will deal with obtaining photons within specified regions of an image. Available regions are: Annulus Box Circle Ellipse Field -- entire field Irregular region based on intensity of map... i.e. region defined by contour levels. ... The imcnts task in the xray-spatial package sums the source and background counts in specified regions, and subtracts one from the other properly normalized. ... imcnts* - Find counts in an extended region, after removing an embedded point source . ...

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• Determine a background subtracted radial profile
• The AstroStat Slog parameter estimation
• Parameters

COS Instrument Handbook for Cycle 24 . ... exposure time . ... overhead times . ... airglow - see background rates . ... apertures 1 , 2 . ... BOA - see apertures, BOA . ... calibration accuracies . calibration observations . ... Cycle 17 calibration observations 1 , 2 . ... detector non-linear effects - see dead time . ... Exposure Time Calculator - see ETC . ... FCA - see apertures, FCA . ... grating parameters . ... PSA - see apertures, PSA . ... spectroscopic modes - see grating parameters . ...

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• Fine Guidance Sensor Instrument Handbook
• Instrumental Parameters
• Index

... Measurement of the MASS detectors parameters with mass program January 24, 2015 [112707] . MASS/DIMM electronics. ... Turbina-core(D): Dimm User Guide. ... N.Shatsky, V.Kornilov, The revision of the MASS/DIMM star catalogue. ... О.Возякова, В.Корнилов, Н.Шатский, Новое программное обеспечение прибора MASS/DIMM. ... V.Kornilov, N.Shatsky, S.Potanin, O.Voziakova, B.Safonov Preliminary results of astroclimate parameters measurements at the Sternberg 2.5m telescope installation site. ...

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... 5 1/ 2 Closing the feedback lo op: 1st option · Feedback efficiency 2NepEep f = Lp 4 3 w1 R 3 E1 w2 c E2 ( Eep E1 if E1 E2) · Pair pro duction rate Nep = · Soft (synchrotron from secondary pairs ) photon field: Eep 2 eB E2 1/2 f w w b , w2 = Es = 4 Es 2 mec2 mec · Hard ( inverse Compton from primary pairs ) photon field: 2 2 wb 3 R w1 , E1 = 3 2Ts wb = 4 R T ct 0 0 mec2 wb is thermal background energy density ...

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The reduction of a given magnitude m to it is given by: . ... The galaxy extraction was made with a Discriminant Analysis based on seven parameters (peak intensity over area, Mean surface brightness, Peak intensity, Axis ratio, Relative surface object/matrix, Elongation of the matrix and Diffraction cross) and calibrated with a sample of 1146 DENIS objects visually classified as "galaxy", "star" or "unknown". A visual inspection of every galaxy candidate was made on the matrix of pixels. ...

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• HyperLEDA documentation: parameter: vdis
• Documentation: LEDA: parameter: v3k
• Command Syntax

... Driver ID: LOCAL . This is a hack to allow a machine to use its own system clock as a reference clock, i.e., to free-run using no outside clock discipline source. ... Another application for this driver is if a particular server clock is to be used as the clock of last resort when all other normal synchronization sources have gone away. ... This driver provides a mechanism to trim the local clock in both time and frequency, as well as a way to manipulate the leap bits. ... Not used by this driver. ...

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• GIMP animations: merge-anim example 1
• CREATE FULLTEXT CONFIGURATION
• FTS Dictionary Example

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
• PPEUC Programme - Cosmic Microwave Background Workshop
• Supernova Remnant (SNR) Catalogue or Catalog of Galactic SNRs

... Forum: The Linux Kernel Hackers' Guide . Keywords: kernel tuning, file handles, Bus error . ... In a recent comp.os.linux. article I saw a reference to tunable kernel parameters, which I think may help me with a problem I'm having with expireover on a Debian 1.2, Inn 1.4 unoff4 news server. ... I'm runnming 2.0.27, 64mb ram, raid 0 on three 2gb drives for /var/spool/news. ... I've been looking for some docs on tuning kernel parameters like file handles, and can't seem to find it. ...

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• Determination of the Detector Parameters
• mod_session_crypto - Apache HTTP Server
• Program parameters

... RC0133+0459 . ... RC0154+0459 . ... Radio source parameters . R.A.(J2000) Dec.( J2000) R.A.(B1950) Dec.( B1950) Freq. Comp. ... MHz] size["] flux[mJy] ["] index 01:54:47.65 +04:59:23.9 01:52:11.19 +04:44:42.1 1425.0 .6 84 - 1.01 . Parameters of optical candidates for identification . ... B1950) Magn. 01:54:47.65 +04:59:23.7 01:52:11.18 +04:44:42.0 22.6 . Cross marks radio source ps . Last updated 20 Dec 2000 ...

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... Of the 4 buttons in the bottom part of the configuration screen, three deals with power level adjustments: the 'Power control' button brings up the power control window where You can adjust the power levels of the different parts of the IF/LO system, the 'Power levels' button brings up the power level monitoring window (which also can be run outside CIMA as the 'powerwin' program), and the 'Adjust Mock power' button which adjusts the power levels on the Mock spectrometer (but nowhere else). ...

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• Nominal Parameters of Galactic Plane Survey
• The CIMA ALFA Instrument Monitor Window
• pdev_birdies_25jun07

... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...

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• Instance-Based Machine Learning Methods for the Prediction of Stellar
• An Object Oriented Design for Monitoring the Chandra Science Instrument X-ray
• A New Entropy Measure Based on Multiple Resolution and Noise Modeling

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Here we present the ionospheric parameters variations for quiet conditions. ...

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• East Siberian Center for the Earth's Ionosphere Research. Specific character
• East Siberian Center for the Earth's Ionosphere Research. Modelling, secondary
• East Siberian Center for the Earth's Ionosphere Research. Capabilities and