... The standard lbn cal diode was compared to the standard diode. Using the standard diode value and the insertion loss the lbn cal value was computed every 25 MHz from 1200 MHz to 1600 Mhz. ... After the measurement, the insertion loss from the standard diode to the output of the coupler was measured over the frequency range 1200 to 1400 Mhz. ... The major uncertainty in the measurement is in the standard diode ENR and the insertion loss of the waveguide transition. ... freq [Mhz] . ...

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• http://www.naic.edu/~phil/callbn/lbSefdGT_Aug00.html
• http://www.naic.edu/~phil/calsbh/meascalMar04/measCalmar04.html
• http://www.naic.edu/~phil/calcb/meascalMay03/meascalMay03.html

... 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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Ref: ALMA band 1 horn measures Date: 27/08/2002 Technical note ALMA band n.1 horn measurements Author: Renzo Nesti Summary This document is intended to give pattern and return loss measurements of the ALMA band n.1 horn (31.3-45 GHz) produced by CLOEMA and designed by MECSA and Arcetri. ... Because the measurements have been made by rotating the horn under test on the expected phase centre we conclude that the estimation of the phase centre position does agree well with tests. ...

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• http://www.arcetri.astro.it/~nesti/pdfs/ALMA%20band%202%20horn%20measures.pdf
• I need some way to measure the time a process spend in READY QUEUE

... The visible power a source emits in all directions is measured in lumens. ... Solid Angle- . ... The solid angle of a light cone is the projected area of the cone divided by the total surface area of the sphere. A solid angle is measured in steradians, where 1 steradian corresponds to the solid angle su btended by a cone of unit slant height and unit projected area. ... Luminous intensity is the flow of luminous energy, or lumens, per steradian. ... This is the rate of flow (lumens) per unit area. ...

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• Armagh Observatory
• Measuring Internet Access
• Measuring Holes

... This paper presents an overview of the CENTERFIT image centering algorithm library currently under development in the IRAF system. ... The centering algorithms employed by these applications must satisfy a wide range of efficiency and accuracy requirements, and function robustly on data sets spanning a broad wavelength, resolution, and signal-to-noise regime. This paper presents an overview of CENTERFIT, a library of 1-D and 2-D centering algorithms currently under development in the IRAF system. ...

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• ADASS 2003 Conference Proceedings
• Simulation of HST PSFs using Tiny Tim
• A New Entropy Measure Based on Multiple Resolution and Noise Modeling

... STIS . ... In a space environment, CCD detectors accumulate radiation damage, which over time leads to increasing dark current, more hot pixels, and reduced charge transfer efficiency. After twelve years on orbit, the effects of such radiation damage on the STIS CCD have become substantial. ... Since in a CCD, charge must be transferred many times before reaching the readout register, even a small decrease in CTE can have a large effect on the measured count rate near the center of the detector. ...

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• Standard Patterns for Substepping and Background Measurement
• Gaps in the Cloud Cover? Comparing Extinction Measures in Spiral Disks
• Measuring Extinction Curves of Lensing Galaxies

Microsymposium 34, MS058, 2001 ANOMALIES OF THE MOON'S THERMAL EMISSION IN THE IR SPECTRAL RANGE (10.5 - 12.5 micron). ... Sternberg State Astronomical Institute, Moscow, 119899, Russia, pugach@sai.msu.ru Summary: New satellite measurements of the lunar-surface radiation temperature were used to construct the spatial angular function of thermal radiation of the Moon in the infrared (10.5-12.5 micron) spectral range. ... These thermal anomalies are observed only in the limited range of phase angles. ...

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• http://selena.sai.msu.ru/Symposium/ir_luna_e.pdf

... Posts tagged ?Differential Emission Measure? ... Differential Emission Measures (DEMs) are a summary of the temperature structure of the outer atmospheres (aka coronae) of stars, and are usually derived from a select subset of line fluxes. ... Continue reading ?Differential Emission Measure [Eqn]? Tags: DEM , Differential Emission Measure , EotW , Equation , Equation of the Week , stellar coronae . ... vlk on [MADS] Parallel Coordinates . upvc windows on [MADS] Parallel Coordinates . ...

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• The AstroStat Slog Blog Archive Differential Emission Measure [Eqn]
• The AstroStat Slog DEM
• The AstroStat Slog stellar coronae

... Class . Use . ... Packages that use Measurements . ... Uses of Measurements in ij . Classes in ij that implement Measurements . ... This is an extended image class that supports 8-bit, 16-bit, 32-bit (real) and RGB images. ... Classes in ij.gui that implement Measurements . ... Classes in ij.macro that implement Measurements . ... Implements ImageJ's Process/Enhance Contrast command. class . ... This plugin implements ImageJ's Analyze/Measure and Analyze/Set Measurements commands. class . ...

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• Uses of Package ij.measure (ImageJ API)
• ij.measure (ImageJ API)
• ij.measure Class Hierarchy (ImageJ API)

... The described algorithm is suitable for measurements of complex images of stars. ... a) the zero-based number of stars in the complex (multicentric) image, . b) set of preliminary coordinates - x i , y i , for all stars, index i is number of a star, . ... i - index of a star in the complex image; . ... These parameters are calculated by a nonlinear method of a least squares.The main output parameters of this algorithm are x i , y i ; where the index i is number of a star in the multicentric image. ...

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... The Science Operation Department is composed of Astronomers, Telescope Instruments Operators(TIOs) and Data Handling Administrators(DHAs). ... Astronomers have proposed several methods to quantitatively measure the amount of turbulence above the telescope, which the most common ones is Differential Image Motion Monitor (DIMM). In optical testing, the Hartmann test is the common method to test the quality of optical components. ... Hartmann mask consists of 48 lenses. ...

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... Science User Portal . ... ESO, the European Southern Observatory . ... Travel and Contacts . Travel to ESO Headquarters . ... ESO . ... Survey Telescopes . ... Galaxies . ... Star Clusters . ... Stars@ESO . ... ESO Science Newsletter . ... ESO 3.6-metre telescope . ... Astronomers using ESOтАЩs Very Large Telescope (VLT) have measured the distance to the most remote galaxy so far, UDFy-38135539, which we see as it was when the Universe was only about 600 million years old (a redshift of 8.6). ...

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• Zooming in on the most distant galaxy ever measured | ESO United States
• Zooming in on the most distant galaxy ever measured | ESO Ireland
• Zooming in on the most distant galaxy ever measured | ESO Australia

... An OBJECT column gives the name of the object observed (usually a star name). ... In critical cases, it is common practice to measure sky on two or more positions around a target object, and these positions must be identified. ... A general treatment of this problem requires a column called OBJECT, bearing the usual name of the object (as in the star tables); a column labelled STARSKY, to distinguish between star+sky, star alone, or sky alone; and additional columns to identify the sky position. ...

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• Measuring aperture
• Columns REDLEAK, RLTYPE, and MAKER
• What was the measurement?

This lesson introduces you to the different types of uncertainty, and how you can estimate them from the scatter in your measurements, or from knowledge of your experimental set-up. It also outlines how to quote uncertainties. Back Main Uncertainties Page .

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• Lab Skills Video Tutorials: Uncertainties

... Optical constants of Fe 2 O 3 in the infrared spectral region. ... Optical constants: . amorphous Fe 2 O 3 . ... The Reflectance of polarized radiation at the incidence angle 12 deg was measured in the range from 1400 to 200 cm -1 for monocrystalline hematite (alpha-Fe 2 O 3 ) and amorphous Fe 2 O 3 samples. Special technique applied allowed to reduce the relative errors downto 1% for the reflectance values of 0.005-0.8. The optical constants were obtained by the Kramers-Kronig method. ...

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• Database of Optical Properties -- Level: subsubpage
• T-matrix method (EBCM)

... Studies of the pathlength fluctuations through the troposphere using geostationary satellite. ... Relationships that connect the temporal structure function of fluctuations measured with the temporal spatial structure functions of pathlength through the troposphere were obtained. ... On the base of experimental data there were determined the parameters of temporal structure function of pathlength through the troposphere (exponent, structure coefficient). ...

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• Keywords_3
• Keywords_340

INFRARED FOURIER-SPECTROMETER SICH-F . ... Instrument work regimes: 1) Inside. 2) Calibration at inside standard sources 2 - 4 times per a rotation. 3) Calibration at "free space" 2 - 4 times per a rotation. 4) Infrared radiation measuring 10 - 40 min. per a rotation. ... Spectrometer consists of the photodetector block and the block of signal processing and control. ... Diagnostic information and attach data will transfer by state telemetric channels. ... Detector temperature. ...

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• EUV PHOTOMETERS PHEUV
• Laboratory static Fourier-spectrometer
• SPECTROPHOTOMETER FAGOT

... Cell depth measurements . Back-plate hole measurements . ... On May 3, 1994 at the Optical Sciences Center at the University of Arizona, measurements of cell depths and locations of the back-plate holes were made. ... Figure 1: Cell labels and coordinate system for the 2.5-m primary mirror. ... This is within 3% of the design value. ... These are plotted against x. Figure 4: Residual cell depths after removing the design radius of curvature of the back-plate and the mean cell depth. ...

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• TUI:Scripts:Built In Scripts:Telescope:Pointing Data
• ARCTIC Commissioning
• Procedure to Collimate the SDSS 2.5m Secondary Mirror

Once students get the hang of it, they can find and measure the brightness of Delta Cephei in a few minutes. ... of Delta Cephei . ... Oct. ... The following table lists the measurements of Delta Cephei made by one amateur astronomer in autumn 1990. ... 4.0 . ... This activity is a simplified version of one that appeared in Hands-On Astrophysics, a series of activities prepared by the American Association of Variable Star Observers with support from the National Science Foundation. << previous page | ...

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• Astronomical Society
• ASP: There's More to Light Than Meets the Eye
• ASP: A Taste of Real Astronomy ? The ESA/ESO Astronomy Exercises

Phase Retrieval Measurements of Antenna Surfaces Using Astronomical Sources Bojan Nikolic, John Richer, Richard Hills Mullard Radio Astronomy Observatory, Cavendish Laboratory, Cambridge, U.K. Abstract We present a novel technique for accurate measurement of the largescale errors in an antenna surface using astronomical sources and detectors. Out-of-focus images of compact astronomical sources contain a wealth of information about the telescope optics. ...

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• http://www.mrao.cam.ac.uk/~bn204/phd_era/oof/oof.html
• http://www.mrao.cam.ac.uk/~kjbg1/lectures/lect1_1.pdf
• Astrophysics Group SKALA meets LOFAR