The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...

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• Optical constant database - Level: measurement/paper

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Chirp ionosonde main technical characteristics . ... Linear frequency modulated continuous signals sounding method is relatively simple and has wide application in various special-purpose systems. ... Chirp signals which are applying for ionosphere channel diagnostics usually have10KHz/s -- 1MHz/s. We must point out that under modulation speed increasing there is an increase in noise suppression and resolution power. ...

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• East Siberian Center for the Earth's Ionosphere Research. Objectives.
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• East Siberian Center for the Earth's Ionosphere Research. Incoherent Scatter

... These electrons may be free or bound to an atom or ion. ... The modelling of a stellar atmospheres (or any astrophysical object) and its emergent radiation requires a detailed model of how photons interact with electrons. ... These "atomic data" are fundamental to accurate astrophysical modelling. ... For calculating model spectra of early-type helium stars in LTE, I maintain a database of atomic data for, mostly, blue-visual absorption lines of light elements. ... Simon's home page . ...

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• Atomic data for Stellar Atmospheres: lte_lines
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• Meteors in Planetary Atmospheres

Subject, Problems and Objects of Theoretical Astrophysics. ... Stellar Photospheres, Their Features. ... Physics of Continuous Radiation Absorption in Stellar Photospheres. ... Continuous Radiation Absorption in Stellar Photospheres of Various Spectral Classes. Solar Type Photospheres. ... Characterisics of Absorption Lines. ... Interstellar Absorption Lines, Their Features. ... Physical and Dynamic Features of Interstellar Medium, Which Follows from Observations of Interstellar Absorption Lines. ...

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• Additional Parts of Theoretical Astrophysics
• HIGH RESOLUTION IONOSPHERIC MASS SPECTROMETER P-11

... On-line calibration consists of calibration operations performed to maintain the ALMA observing system properly tuned to successfully execute the planned observations. ... Among processing operations are the calibration of the atmospheric absorption, of phase radiometric correction, of pointing scans, of phase and amplitude reference measurements, .. ... In the mean time tests of the calibration software will proceed using both simulated data and data from the antenna prototypes...?re 1 . ...

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• ADASS 2002 Conference Proceedings

Next: Computation Up: userhtml Previous: Restoring an image . Because the basic interpolated calibrator gains do not determine the antenna gains perfectly at each time stamp, the quality of the resultant image suffers. Often the technique of self-calibration is used to make additional corrections to the antenna gains as a function of time. ... The main difference is than the model of the source is generally more complex than just assuming it's a point source at the phase centre. ...

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• An alternative approach to calibration
• Frequency Handling
• Bandpass and antenna gain calibration

Next: CONCLUSION Up: CHIRPLET TRANSFORM SUBSPACES Previous: Nondilational Chirplet Transform . Suppose we choose a windowed sinusoidal FM signal for our mother chirplet. Such a signal has a frequency that periodically rises and falls (much like the vibrato of musical instruments or the wail of a police siren). ... Figure 14 . ... Using the warbling mother chirplet, we also computed the ``dilation-dilation'' ( ) plane of the chirplet transform (Fig. 16 ) for the pendulum data. ...

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• Time-Frequency-Scale Volume
• THE CHIRPLET

. Departement of Quantum Astrophysics . Head: Kurt V.G. , Prof. ultraviolet spectroscopy of planetary upper atmospheres and interplanetary/interstellar medium; . observations of gamma-bursts and optical identification of their sources; . long-base optical interferometry. Staff: .

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• Description of the RadioAstron project, english version
• RadioAstron Mission Element Overview

... Scattered within this cavernous nebula, cataloged as NGC 604, are over 200 newly formed hot, massive, stars. At 1,500 light-years across, this expansive cloud of interstellar gas and dust is effectively a giant stellar nursery located some three million light-years distant in the spiral galaxy, M33. Hyakutake: Comet Atmosphere . ... The atmosphere of a comet comes and goes. ... Yesterday the Mars Global Surveyor project released a new close-up image of a portion of the Cydonia region on Mars. ...

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Next: Filtering ROSAT HRI data Up: ROSAT HRI Recipes Previous: Correlating Spectral Data with . Although the spatial variation of the quantum efficiency across the HRI is nominally within 10% for most of the detector, occasionally it may be desirable to flat-field a map with preflight calibration measurements. ... Store the new gain map image using ``blink" in SaoImage. ... The quantum efficiency correction (QEC) is the inverse of the intensity determined from the QE map at the source position. ...

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• Calibration
• Correlating Spectral Data with Spatial Gain Variations
• The AstroStat Slog Hubble constant

... public class Calibration . ... static int . ... double . ... Returns true if this image is spatially calibrated. public void setUnit (java.lang.String unit) . ... Converts a z-coodinate in pixels to physical units (e.g. mm). public void setFunction (int function, double[] coefficients, java.lang.String unit) . Sets the calibration function, coefficient table and unit (e.g. "OD"). public void setFunction (int function, double[] coefficients, java.lang.String unit, boolean zeroClip) . ...

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• Measurements (ImageJ API)
• TiffDecoder (ImageJ API)
• RoiDecoder (ImageJ API)

For the calibration of RATAN-600 data you will need to Download Nobeyama Fluxes (1, 2, 3.75, 9.4, 17 GHz): year 1999 2000 2001 2002 2003 . Brief description of Work Scan . Main functions of processing, realized in the program are: . ... Correction of various (not fatal) defects of data; . ... Calculating of the lower enveloping curve or an average scan from observations data for a few days; . ... COMMENT This table contains the set (TFIELDS) of 1-dimensional (TFORM# . ... AZIMUTH = 'float' / . ...

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• RESEARCH PROBLEMS of the LRS
• Cosmological Gene project
• Gazinur Galazutdinov home page

... title=' fashion наручные мужские часы Pierre Lannier 243F033. Коллекция Elegance Basic - Pierre Lannier' border='0' align='left' width='120' style='margin-right: 20px;' hspace='7' vspace='5'/> Кварцевые часы. ... Коллекция: Barete . ... Светильник LSF-7700-01 легко выступит в качестве объекта современного искусства в интерьерах поп-арт, хай-тек или кантри. ... Мужские наручные швейцарские часы в коллекции Timewalker Montblanc - Montblanc - Montblanc . ...

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• Катушка индуктивности Jantzen - Jantzen - Jantzen Ортез на лучезапястный сустав
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• Стойка для бокса Interatletik СТ 801 - Interatletik - Interatletik

... Published spectra . Published k-corrections (Bessel & Brett filters) . K-corrections using CIT filters . Filters used for the integration: U B V Rc Ic J CIT H CIT K CIT . Filters used for the k-corrections: J BB H BB K BB . New calibration of the spectra: set the desidered colors (Johnson BV- Cousins RI- CIT JHK) in the table below, press "SUBMIT" and save the output as text file. ... Spectra of individual galaxies ( calibrated in lambda and flux and normalized to average=1) . ...

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• The Motion of Comets
• Hubble Finds Oxygen Atmosphere On Jupiter's Moon Europa
• Galileo Probe Suggests Planetary Science Reappraisal

The ESA/ESO Astronomy Exercise Series 2 . The Distance to Messier 100 as Determined by Cepheid Variable Stars . ... The small variations in distance to the individual Cepheid variable stars in the Cloud are negligible compared with the much larger distance to the SMC. ... In this way Cepheid variable stars can be used as one of the 'standard candles' in the Universe that act either as distance indicators themselves or can be used to calibrate (or set the zero point for) other distance indicators. ...

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• ASP: AstroCappella - A Musical Exploration of the Universe
• ASP: Taking a Grand Virtual Voyage in the Milky Way
• ASP: Star Science in the Autumn Sky

... Left: A POSSM plot of the uncalibrated spectrum of DA 193 at 1.66 GHz on a baseline Bear Lakes to Noto. ... The phase slope as a function of frequency is clear evidence for a small delay error in the correlator model. Right: The same data as shown on the left, but corrected for a delay error and a residual fringe rate. ... Left: A VPLOT plot of the uncalibrated amplitude (upper frame) and uncalibrated phase (lower frame) as a function of time for the source DA 193 on a baseline HartRAO to Noto. ...

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... It has been largely superceded by MatWeb . Conversion Factors . Material properties . Physical constants . Astronomical constants . This table gives conversion factors to convert various units to their SI equivalents. ... The units are SI. This is a short list of physical constants in SI units. ... Boltzmann constant . ... Gas constant . ... Mass . ... Plank's . ... Radiation constant . ... This is a short list of astronomical constants in SI units. ... Sun . ...

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• TUI:Telescope:Offset Types
• Astrophysical Research Consortium - Apache Point Observatory
• telescope tests

Bigbang Forum Message . Forums: . ... Discussion Forums | ... All True IF Speed Of Light Is Constant (I Can Question That.. Forum List | ... Post Message | ... basicaly it says that speed of light is not constant because it depends of the movement of the source. ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• Brilliant! Thanks - an Astronomy Net Blackholes2 Forum Message
• A Question Of Atmosphere On Our Moon!? - an Astronomy Net God Science Forum

Stellarium 0.12.3 . ... Classes . ... FileљStructure . ... Atmosphere Class Reference . ... More... #include < Atmosphere.hpp > . voidљ . computeColor (double JD, Vec3d _sunPos, Vec3d moonPos, float moonPhase, StelCore *core, float eclipseFac, float latitude=45.f, float altitude=200.f, float temperature=15.f, float relativeHumidity=40.f) . ... Get fade in/out duration in seconds. ... getFlagShow () const . ... getFadeIntensity (void) const . ... Definition at line 40 of file Atmosphere.hpp . ...

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• Stellarium: core/modules/Atmosphere.hpp Source File
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• Twitter Weekly Updates for 2013-09-13

... 2000: . It is shown that radio emission of microbursts in solar active regions is the manifestation of noise storms at the fundamental plasma frequency, and is the result of instabilities propagating at the tops of coronal loops. ... Collaboration with the Nancay Decimetric Radio Telescope (France). A method for determining the height of the corona base above sunspots was proposed. ... Archive . ...

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• New data on the cpmplex field structure of chemically peculiar stars
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