The field-of-view and angular resolution of the wide field and planetary camera is split up as follows (see Chapter 4 for more details on CCDs): . Table 2.1: Summary of Camera Format. Camera . ... Field-of-View . ... Wide Field . 800 800 . ... Planetary . ... 28.3 Figure 2.1: Wide Field Planetary Camera Concept Illustration. ...

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• A Brief Description of the Instrument and Its Operation
• Chapter 2: Instrument Description
• Chapter 2:  Instrument Description

... hkgtigen (hkgtigen-1.14.2) [xmmsas_20080701_1801-8.0.0] . Meta Index / Home Page / Description For each instrument standard HK parameter validity ranges are stored in the corresponding CCF constituent HKParmInt [ 2 ]. The ranges are expressed in terms of boolean selection expressions as defined by the selectlib package. ... In more detail, when invoked for a particular instrument (see parameter instrument ), hkgtigen performs the following operations to construct the single GTI data set: . ...

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• Instrument Details Record

Next: Summary of reduction Up: Echelle Reduction Previous: Saving the Data . In the present version we will be concerned with the standard configuration of CASPEC, the Cassegrain Echelle Spectrograph which is in operation at the Cassegrain focus of the ESO 3.6 m telescope. ... In its standard configuration CASPEC uses a a 31.6 lines/mm echelle grating together with a 300 lines/mm grating cross disperser. ... The table shows the change in resolution with the order number. Table: Resolution . ...

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• Echelle Spectra
• WSRT deep surveys

The following papers summarize the characterization and technical performance of IBIS : . ... Characterization of Fabry-Perot interferometers and multi-etalon transmission profiles. ... Righini, A., Cavallini, F., Reardon, K. P., 2010, Astronomy and Astrophysics , 515 , A85, . ... The filter wheel is located between the two interferometers. ... The interferometers can be rapidly tuned, simultaneously, so to allow sequential scanning of the spectral lines of interest (see movie in IBIS Intro ). ...

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• The LongSp Description
• Venera 12 Descent Craft
• Venera 11 Descent Craft

SHORT DESCRIPTIONS OF INSTRUMENTS . ... Particle detector RIEP-2802 was developed and built in Russia. ... The combined Soviet-French ONCH-TBF onboard instrument had in memory modes the data only from several filter-banks in the range from 10 Hz to 16 kHz (while in the real-time telemetry modes, the measurements included 5-component wave-form data in the range 10 Hz - 1.5 kHz for 3 magnetic and 2 electric field components, or a wide-band mode in the range 10 Hz - 15 kHz, and several filter banks). ...

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• PhSRM
• HYPERBOLOID Results Page
• SKA-3 Experiment Description

... v1.2.3: muc09/10 added; monthly mode for phoenix (mcalib mode) . ... condor concepts | ... This tool visualizes the status of the current condor processing cascade on a MUC blade. ... in DATE mode (-d), it visualizes the latest cascade of that date (or, if -c is used, that specified cascade), in a detailed overview ("high-resolution") . ... The cadence of the tool for the watch mode is configurable and should be roughly adapted to the typical execution time of ABs (usually 30-60 sec is a good value)...

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• pyQC: overview
• CRIRES - VLT High-Resolution IR Echelle Spectrometer
• ESO - Paranal Instrumentation

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Classes . Files . ... All љ Classes љ Namespaces љ Files љ Functions љ Variables љ Typedefs љ Enumerations љ Enumerator љ Macros љ Pages . tcc . InstPosition . ... tcc::InstPosition Class Reference . ... InstPosition (std::string const &name="?") . ... PF1 = prime focus the following require a secondary mirror: . ... BCx = bent Cassegraine foci at top and bottom of mirror cell (when telescope is at horizon) . ... Definition at line 49 of file instPos.h . ...

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• lsst.tcc: tcc::TcsPOrig Class Reference
• MILT Multiple Instrument Large Telescope
• MILT Description

... public class TiffDecoder . ... static int . ... Field Detail public static final int NEW_SUBFILE_TYPE . ... public static final int IMAGE_WIDTH . ... public static final int IMAGE_LENGTH . ... public static final int BITS_PER_SAMPLE . ... public static final int COMPRESSION . ... public static final int PHOTO_INTERP . ... public static final int IMAGE_DESCRIPTION . ... public static final int STRIP_OFFSETS . ... public static final int ORIENTATION . ... public static final int SAMPLES_PER_PIXEL . ...

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• API Help (ImageJ API)

This diagram illustrates the effects of floating a box ("inner") and how its "sibling" is forced below it due to the 'clear' property. A document window is shown, with 8 lines (numbered 1 to 8), each 24px high. Text before the "inner" box flows on lines 1 and halfway on line 2. The "inner" box has been floated to the right and occupies the second half of lines 3 and 4. ... The lines, as they appear in the image, contain: 1 Beginning of body contents. ... Inner contents" is blue. ...

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• Long description illustrating absolute positioning with respect to the initial
• Long description for example illustrating absolute positioning
• Long description of example illustrating floating without clear

... GSAOI Home . Instrument . ... The Gemini South Adaptive Optics Imager (GSAOI) is a near-infrared adaptive optics camera that will be used with the Multi-Conjugate Adaptive Optics (MCAO) system on the Gemini South 8-m telescope . ... Gemini's major instrumentation goal is to develop its Multi-Conjugate Adaptive Optics (MCAO) system for scientific use on Gemini South. ... Existing adaptive optics systems use a single natural guide star or artifical laser guide star to measure this image blur. ...

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• Software Maintenance Manual
• GSAOI Orion Nebula Cluster Science Page
• GSAOI Magellanic Cloud Planetary Nebulae Science Page

Stellarium 0.12.3 . ... Classes . ... FileљStructure . ... Protected Member Functions | ... StelSkyPolygon Class Reference . ... StelSkyPolygon (const QString &url, StelSkyPolygon *parent=NULL) . ... StelSkyPolygon (const QVariantMap &map, StelSkyPolygon *parent) . ... voidљ . ... initFromUrl (const QString &url) . ... initFromQVariantMap (const QVariantMap &map) . ... loadFromQVariantMap (const QVariantMap &map) . ... Definition at line 31 of file StelSkyPolygon.hpp . ... const QString &љ . ...

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• Stellarium: SphereParams Struct Reference
• Stellarium: RingParams Struct Reference
• Stellarium: Nebula Class Reference

Description and Technical Details . In 1980s two medium-size horizontal solar telescopes 50/35000 cm with large spectrographs Czerny-Turner made by Carl Zeiss Jena were installed in the Ondњejov observatory. The Czerny-Turner-spectrographs in the Ondњejov observatory called HSFA1 and HSFA2 according to the German name Horizontal-Sonnen-Forschungs-Anlage ("horizontal device for solar research") have been explored for more than two decades. ... Diffraction grating - Richardson, Spectra-Physics . ...

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• Technical Details

... The Miriad task uvgen can be used to simulate a variety of observing modes. ... Simulating a telescope approximately, let alone in some detail, requires a good many parameters. uvgen takes an appreciable number of parameters and input files to describe the telescope, correlator and source. Fortunately keyword and set-up files for some common situations exist ( e.g. simulating the ATCA and VLA). ... For example, to load typical parameters for the ATCA, use miriad% source $MIRCAT/uvgen.def.atca . ...

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• difx:ivs2016extras [ATNF VLBI Wiki]
• casacore: casa::DOos Class Reference
• casacore: casa::MSSpectralWindowEnums Class Reference

Radar Astronomy Group . ... This instrument will enable the Observatory to detect asteroids over a very much wider radial range than with the old 420 kilowatt system. ... Here are some recent images of asteroids obtained with the Arecibo Planetary Radar. ... The following data were taken by various observers using the Arecibo Observatory 12.6 cm radar. ... Chris De Vries wrote a description of how to reduce planetary radar data , using the 1988 Venus data taken at the Arecibo Observatory as a model. ...

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• Pulsar Instrumentation the Arecibo Observatory
• Project Description
• Chapter 13. Configuring TwinView

... Up: Telescope and Instrument Control Systems . ... 216, Astronomical Data Analysis Software and Systems IX, eds. N. Manset, C. Veillet, D. Crabtree (San Francisco: ASP), 271 . ... NASA Goddard Space Flight Center and AppNet, Inc. are developing AIML to command and control astronomical instruments. Our software architecture combines the platform-independent processing capabilities of Java with the power of XML. ... Instrument description is too tightly coupled with details of implementation. ...

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• System Interfaces to the STIS Calibration Pipeline
• Calibration and Performance Control for the VLT Instrumentation
• NASA's Instrument Control Markup Language (ICML)

... Status of the ELECTRON experiment . ... The objective of the ELECTRON experiment is to perform 3-D measurements of the plasma electrons in the energy range from 10 eV to 26000 eV, with good angular resolution, sensitivity and large dynamical range. ... Figure 1 presents the ELECTRON sensor. ... Click on the picture to view large one) . ... Figure 3 shows dynamical spectra with counting rate measurements performed by ELECTRON experiment during very multiple magnetopause crossings on February, 4, 1996...

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• Sensors
• OMNIDIRECTIONAL PLASMA SENSOR VDP
• THE LOW ENERGY PLASMA COMPOSITION EXPERIMENT AMEI-2

STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... Telescopes . ... Superb optical performance coupled with time proven computerized pointing and tracking has made the LX200 ACF series a best-seller in the high-performance telescope class. ... Series 6000 APO Refractors . ... These telescopes come with all necessary equipment in the box and feature an altazimuth mount that allows for easy and quick viewing. ... NG70-SM Altazimuth Refractor . ... Meade NG70-SM Altazimuth Refractor #20218. ...

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• Meade Series 4000 #3200 Lunar And Planetary Color Filter Set
• WildernessтДв Binoculars - 8x42
• WildernessтДв Binoculars - 8x25

... The TESIS is a set of solar imaging instruments developed by the Lebedev Physical Institute of the Russian Academy of Science, and launched aboard the Russian spacecraft CORONAS-PHOTON on January 30, 2009. The main goal of the TESIS is to provide complex observations of solar active phenomena from the transition region to the inner and outer solar corona with high spatial, spectral and temporal resolution in the EUV and Soft X-ray spectral bands. ... Solar activity hits a new low . ...

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• TESIS

Main Page Data Structures File List Data Fields Globals . Data for OI_WAVELENGTH FITS table. ... int . ... char . ... float * . eff_wave . ... eff_band . Data for OI_WAVELENGTH FITS table. int _oi_wavelength::revision . char _oi_wavelength::insname[FLEN_VALUE] . int _oi_wavelength::nwave . float* _oi_wavelength::eff_wave . float* _oi_wavelength::eff_band . The documentation for this struct was generated from the following file: . ...

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• DUST: Dust::TUpwardLimInt Class Reference
• DUST: dust_EBins Struct Reference
• DUST: Dust::PowerOutInt Class Reference

... Average resolution at altitude H=668 km . ... Swath width at H=668 km and inclination of beginning of swath 20.48 degrees . ... Resolution at H=668 км . ... Наименование параметра . ... 1 канале . ... Полоса обзора при H=668 км . ... 1-5 спектральной зоне, не более . ... 1 спектральной зоне . 0,48-0,52 мкм . ... 0,915-0,997 мкм . ... 1-4 канал . ... 1-4 каналов . ... Спектральные характеристики каналов (по уровню 0,5): . ... For more information send a mail to: info@sputnik.infospace.ru . ...

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