. Please find the ASCII files descriptions as follows: . Multisatellites magnetic conjugations (controlled by the 'cnj' button); . Four satellite coordinates (controlled by the 'bl4' button).

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• The FSP ASCII file description
• HYPERBOLOID Results Page
• ASCII files description

Ground Support of RadioAstron . Control and Tracking Stations . RadioAstron satellite control (command transmission, telemetry, orbit measurements) will be conducted from Evpatoria and Bear Lake control stations. ... Coarse orbit measurements will be carried out from control stations. Each measurement takes ten minutes. ... Orbit measurements at tracking stations give only radial component of spacecraft velocity but the measurements are going continuously during observing sessions. ...

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• Description of the RadioAstron project, russion version

. You can get a short description of each ftp command by typing help followed by the command you want to know more about and pressing the <RETURN> key. For example: ftp> help open open connect to remote tftp ftp> . If you find this description is too brief you will find a much fuller one for each command in the Unix Programmer's Manual pages for ftp .

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• rtftohtml Users Guide - 7 Nested Lists
• HTML Math
• The Structure of HTML 3.0 Documents

... Star Atlas . ... stars . ... If neutron stars don't produce energy from fusion, like normal stars, how can they shine in visible light? ... Although it is true that neutron stars have, for the most part, consumed all their internal thermonuclear fuel, they tap into other energy sources to produce light. Indeed, neutron stars are remarkably "resourceful" and employ a variety of physical mechanisms to make themselves visible.A newborn neutron star is incredibly hot ? ... Atlas of the Stars . ...

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• Spectacularly bright object in Andromeda caused by "normal" black hole |
• Astronomy Magazine - Interactive Star Charts, Planets, Meteors, Comets,
• NASA's New Horizons to return to normal science operations after spacecraft

... Кресла . ... Размер: XS . ... Цвет: белый . ... Размер шлица: PZ2 ; . ... Цвет: Фиолетовый . ... Глубина: 90 . ... Цвет: черный . ... Цвет: серый . ... Размер INT: 54 . ... Глубина пропила: 90, . ... Макс. глубина пропила под углом 90?: 90, . ... Размер площадки: 800x550, . ...

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• Одеяло Сонный гномик Сердечко 90 х 90 см голубой хлопок 588 - Сонный гномик -
• Брюки Saint Tropez Модель: 26474651 - Saint Tropez - Saint Tropez Юбка Motion
• Настенный светильник Favourite Espresso 1503-1W Панно "Буква 'O'

... Mars to Appear Normal this August . ... October is the best month to see Mars this year. ... As Earth catches up to Mars in their respective orbits around the Sun, Mars will keep rising earlier in the night. On 2005 October 30, Earth will have caught up to Mars and the planets will be the nearest to each other in their orbits -- this time around. On October 30, Mars will be nearly opposite to the Sun, rise at sunset, set at sunrise, and appear highest and brightest around midnight. ...

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• Астронет > Mars to Appear Normal this August
• Journal "Peremennye Zvezdy"
• XWare > APOD

... This API (Application Programming Interface) document has pages corresponding to the items in the navigation bar, described as follows. The Overview page is the front page of this API document and provides a list of all packages with a summary for each. ... Each package has a page that contains a list of its classes and interfaces, with a summary for each. ... Each of these pages has three sections consisting of a class/interface description, summary tables, and detailed member descriptions: . ...

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• dec drive adjust

Pulkovo Photographic Plate Database . To find a certain plate, type its number, choose instrument and click button FIND Instrument: Normal Astrograph 26-inch refractor Plate number: . To find plates with a certain sky area: choose instrument, type coordinates (R.A. and Dec.) of the center of this area, type radius of this area, type (optionally) names of required objects, and click button FIND . ...

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• Pulkovo Databases

... The words are numbered according to the reference mentioned above. ... 59 WORD wSecond ; // 0 .. 59 satellite tracking start time (GMT) float fStep ; // reserved WORD wMass ; // reserved BYTE reserved [12] ; // reserved WORD wExtraBytes ; // reserved } TRAJECTORYHEADER ; NOTE: the satellite tracking start time is a hardware operating start time to follow satellite. typedef struct { // ephemeris at satellite tracking start time double time ; // Epoch time (yyddd.ddddddddd)...

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... SIXA FM ACCEPTANCE TESTS . ... In accordance to plan of the Acceptance Tests for Flight Models which was agreed in March 2000 in Moscow, the Acceptance Test of SIXA FM was carried out between 28 August and 2 September at VTT Automation, Finland. ... GOUCH for electronics box of SIXA-FM, Remark: not updated after changes made in 1994. ... Ground Test Program of SIXA-FM. ... Integration Test of SIXA FM, BIUS, ISS, DSS, and MPMI . ... Test data were written to MPMI, DSS-F, DSS-S and GSE SIXA-FM, . ...

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• RTT150 Technical Description

. Home . Structure of Data . Description . Catalog . Publications . VO . ЮБ 2000 . 11:14:20.2 . ЮД 2000 . -57:33:04 . l . 290.172 . b . 2.895 . diameter . 14.0' . (m - M) 0 . 11.4 0.05 . distance . 1900 50 pc . E(B - V) . 0.08 0.01 . log(t) . 9.65 0.05 . (J, J-H) isochrone VOTable . 2MASS data VOTable . Developed by the Team . Send us your questions or feedback

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• SAI OCL Catalog Czernik 23
• SAI OCL Catalog Czernik 21
• SAI OCL Catalog Berkeley 97

... A scan of the superconductor-nonsuperconductor transformation in single crystals of YBa 2 Cu 3 O 6 + x ( x 0.37) is done in two alternative ways, namely, by applying a magnetic field and by reducing the hole concentration through oxygen rearrangement. The in-plane normal-state resistivity a b obtained in the two cases is quite similar; its temperature dependence can be fitted by a logarithmic law in a temperature range of almost two decades. ...

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• Interacting Electrons in Normal Metals
• Theoretical department of ISSP RAS
• CdWO4 Safety Data Sheet

... 1995: . ... for the first time a magnetic field was registered on normal white dwarfs. ... A study of variability of the first galactic superluminal radio source GRO J1915 +10 with the RATAN-600 showed a delay of flare activity at 3 frequencies of 5-10 days after the X-ray flares with an inversion of the radio spectrum. ... The distribution of linear dimensions of clouds in the first approximation is power-law. The distribution of clouds by concentrations depends on the galactic latitude. ...

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• Preparing and Submitting Tabular Data

... Information about a variety of different calendars for different cultures (e.g., Christian, Jewish, Muslim, Chinese, Hindu etc.) ... In addition, the Chinese had two different ways of interpreting and observing celestial events. One way the Chinese used astronomy was known as lifa; it was a discipline that aimed to understand the regularities and the predictable events in the celestial system through careful, observations, measurements and records. ... back to Teachers' Newsletter Main Page ...

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• ASP: The topsy-turveying of planets, stars, and lava lamps
• ASP: Making Your Own Astronomical Camera
• ASP's 119th Annual Meeting - Conference Proceedings

def DER_SNR ( flux ): # ===================================================================================== DESCRIPTION This function computes the signal to noise ratio DER_SNR following the definition set forth by the Spectral Container Working Group of ST-ECF , MAST and CADC. signal = median ( flux ) noise = 1.482602 / sqrt(6) median ( abs (2 flux _i - flux _i-2 - flux _i+2)) snr = ...

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• Space Telescope-European Coordinating Facility
• POLIMODEL (V1.00) --- April99 --- POLIMODEL (V1.00)
• DER_SNR: A simple and general spectroscopic signal-to-noise measurement

... Wavelength Calibration . ... 30s wavecal plot . 30s flatfield plot . ... HeNeAr 4400 . B rQrtz 4400 . ... HeNeAr 4500 . ... BrQrtz 4200 . BrQrtz 4500 . ... These figures in the above table show the number of counts received from each of the lamps in a 30 second exposure with the 1.5 arcsec slit. ... Users have the option of taking calibration lamp data at the rotator angle of each object, but in many cases, it should be possible to measure the shift using observations of night sky lines. ...

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• TUI:Instruments:DIS:DIS window
• lsst.tcc: tcc::InstPosition Class Reference
• MILT Description

The most recent kpyymm.tab (yymm stands for year and month, each expressed with two digits) files are distributed per e-mail half-monthly by Dr. H.-J. Linthe, mailto:kp_index@gfz-potsdam.de Both recent and past tables are supplied as an archive on the FTP servers . ... Since many observatories are interested mainly in the international quietest and most disturbed days, beginning August 1996 three extra lines have been added to the end of the table containing these values in an easy to read form. ...

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• OMNIDIRECTIONAL PLASMA SENSOR VDP
• Influence of onboard events onto spin parameters
• NAIF IKI Home Page

... N. Christlieb 1 and L. Wisotzki . ... We report on the software system L INN ?, which has been designed for the development and evaluation of classification models. ... A few years ago we started to develop methods for the systematic exploitation of the stellar content of the survey by means of automatic spectral classification. ... In this paper we report on the software system L INN ?, that has been designed for the development and evaluation of classification models. ... Class definitions . ...

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• Modelling Spectro-photometric Characteristics of Eclipsing Binaries
• Object Detection Using Multi-Resolution Analysis
• Automated Spectral Classification Using Neural Networks

... Image created from the following: 120 images of Clear filter, 20 of RGB. each of 60 second subframe. 10 Haplha of 120 second subframe. Combined Red and Halpa to get a red/haplha mean image and then processed normally through CCDStack with finishing process through Photoshop CS 5. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

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Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... The algorithm and appropriate program for decametric radiosignal propagation conditions prediction for paths from 500 to 9000 km have been developed at ISTP SB on the basis of normal wave method (AltyntsevaB.I,Iliyin N.V., Kurkin V.I. and others //Decameters channel simulation on the base of normal wave method . ... Solar activity indices are chosen automatically from the prediction date from the database . ...

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