RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . ... SSRT - Receiving systems . The SSRT has two independent receiving systems for recording solar observational data, and several ancillary receivers for checking, setting up and adjusting the instrument. The base receiving systen is a multichannel filter receiver for a simultaneous recording in 180 channels with the 500 kHz band each, adjusted at steps of about 600 kHz. ... Channel's band . ...

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Stellarium 0.12.3 . ... Classes . ... ClassљList . ClassљIndex . ... TuiNodeDouble Class Reference . Allows navigation but also editing of a double value. ... TuiNodeDouble (const QString &text, QObject *receiver, const char *method, double defValue, double min, double max, double inc, TuiNode *parent=NULL, TuiNode *prev=NULL) . Create a TuiNodeDouble node. ... virtual TuiNodeResponse љ . ... TuiNode (const QString &text, TuiNode *parent=NULL, TuiNode *prev=NULL) . ... virtual TuiNode *љ . ...

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• Stellarium: TuiNodeInt Class Reference
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Towards celestial sources above 1 THz with a heterodyne receiver based on a hot-electron bolometer mixer Sergey Ryabchun, Ivan Tretyakov, Matvey Finkel, Natalia Kaurova, Boris Voronov and Gregory Gol'tsman HOT-ELECTRON BOLOMETER (HEB) MIXER Scient ific and Educatio nal Radiophysics Center Mo scow State Pedago gical University Mo scow, Russia FIRST GROUND-BASED OBSERVATION WITH HEB MIXERS BEYOND 1 THz Submillimeter Telescope ...

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• http://site2010.sai.msu.ru/static/doc/Site2010-Summary.pdf

... The reduction system of observations FADPS (description in Russian) (Flexible Astronomical Data Processing System) for data of wide-band receivers of the first observation cabin of the radio telescope RATAN-600 had been created under the Unix-like operational system DEMOS for computers of the SM-1420-type (PDP/11) in 1987 for observation analysis and estimates of coordinates and flux densities of radio sources. ... FADPS: flexible astronomical data processing system at RATAN-600 in UNIX environment....

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The most up-to-date information related to atmos 3.0 are collected here due to constantly increasing interest to MASS/DIMM processing software... atmos 3.0 is still beta , so the latest version is 2.97.5 (there is also 2.98.x branch which absorbs new features) . ... M' line: . ... free seeing and its relative error . ... dimm seeing and its relative error (if dimm data are present, zeros otherwise) . ... dimm turbulence power and its relative error (if dimm data are present, zeros otherwise) . ...

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... All circuit parameters have been presented in a symbolic form. ... To use the program you will need a CIR file (PSpise, DesignLab file) of your circuit. CIR file examples have been enclosured: bpasside.cir, test1.cir, test2.cir, test3.cir, test4.cir, laksamp.cir, bridge.cir, uA741acf.cir, quartz.cir. ... Ideal operational amplifier (nullor) * Nname n1 n2 n3 n4 * * In the ideal op amp data, (n1,n2) represent output nodes, * (n3,n4) represent input nodes (noninverting, inverting). ...

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Due to technical issues, on September 11, 1998 the radiolink was switched to 465 MHz channel. Data acquisition is presently performed only by SRC "PLANETA", Data Receiving Center in Obninsk and Western Siberia Data Receiving Center in Nobosibirsk . For conditions of obtaining data from RESURS-01 N3 please contact SRC "PLANETA". ... Registration of full data stream (61.44 Mbit/s) is performed only by Data Receiving Center, SRC "PLANETA", Obninsk. ...

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• PLANETA home page

Astronotes Armagh Planetarium's Stellar Blog! ... Armagh Planetarium . ... Space Flight . ... By admin December 16, 2015 Posted in: Armagh Planetarium . There have been so many fantastic entries this year that the judges have struggled to pick the winners, so in the spirit of Christmas we now have four overall winners that have won a trip for their class to come to the planetarium and 28 runners up who have each won an individual family pass to visit the planetarium! ... Subscribe to Astronotes . ...

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• Booking | Armagh Planetarium Events
• BBC Stargazing | Armagh Planetarium Events
• BBC | Armagh Planetarium Events

. Please enter the lightcurve FITS file name: . Lightcurve file: . Please note, the output dates are Barycentric-corrected Julian Dates expressed in Terrestial Time - BJD(TT). A similar FITS-to-ASCII lightcurve converter is available for SuperWASP data. If you have questions, bug reports or suggestions how to improve this service, please fell free to contact the author (Kirill Sokolovsky) via e-mail: kirx[at]scan.sai.msu.ru .

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• VaST homepage

... Telescopes . ... The spectrograph is installed in the Nasmyth focus of the BTA telescope, the equivalent focal length is 186 m (F/31). ... The preslit device unit is marked by number 3. ... Fig. ... slit unit of the MSS, 4.1 ? ... The spectrograph slit unit consists of a mirror that redirects the light beam from the Z axis and from the calibration path at an angle of 65њ to the axis of the telescope focus into the slit, the order separation filter, the block of the slit and the shutter (Item 4 in...

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• GRB090726
• Electronic version of Russian Bulletin
• Zeiss-1000 telescope application form

set timefmt '%Y-%m-%d %H:%M:%S' set xdata time set title 'MASTER-NET CGRaBS J0211+1051 Unfiltred observation' set ylabel 'Magnitude' set xlabel 'Time' set term gif set output 'lc.gif' set yrange [] reverse unset key set format x '%Y' set grid plot 'lc.cat' u 1:4 w p notitle , 'lc.cat' u 1:4:5 w errorbar

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• http://observ.pereplet.ru/images/Parasyte.cfg

. S. G. Pugacheva and V. V. Shevchenko, Sternberg State Astronomical Institute, Moscow University, 13 Universitetsky pr., 119992 Moscow, Russia, pugach@sai.msu.ru . Pugacheva LPS 41.pdf - 208K б . Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow, 119992 Russia . Received December 21, 2009 . SSR-10(Busarev).pdf - 239 KB . V. V. Busarev . Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow, 119992 Russia . Received December 21, 2009 . SSR-11(Busarev).pdf - 204 KB .

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• Бережной А.А.
• Aleksei A. Berezhnoi
• Geophysical Research Abstracts

... Здесь собраны функции, необходимые для работы программы. #ifndef VIGG0_H #define VIGG0_H int FindMatrix( string InputString, string SearchString1, string SearchString2); void Invert ( string In); void ComplementaryStr( string In); void Swap( string objA, string objB); class Integer_Node { int Node_handles; Integer_Node * Node_next ; public: Integer_Node( int new_carry): Node_handles(new_carry), ... NO=0)\t"; cin>>ComplementScanActive; cout<<"Want new locus scan start signal? ...

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