Beginning from the May of the 1997 we started to publish our daily solar radio observations at RATAN-600 radiotelescope. ... Periscope System: South Sector+Flat Mirror . ... It is possible to track a source by moving the secondary mirror along the arc-shaped railway tracks or to perform azimuthal 2D map synthesis . ... 1) It is possible to simultaneously carry out independent observing programs using individual sectors at various discrete azimuths and secondary mirrors on corresponding railway tracks. ...

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• Feed cabine #1 for continuum observations
• Feed cabine #3 for solar observations
• Spectrometric complex LRS

RESULTS OF THE PROMINENCE OBSERVATIONS AT MICROWAVES DURING THE MAXIMAL PHASE OF THE TOTAL SOLAR ECLIPSE OF MARCH 2006 O.A. Golub china, V.M. Bogo d, A.N. Korzhavin, N.N. Bursov, S. Kh. Tokhchukova SPb branch of SAO RAS, St.Petersburg, Russia oag@OG4466.spb.edu Results of the prominence radio emission study according to observations of the solar eclipse on 2006 March 29 with the Northern sector and with the Southern sector with the Flat mirror of RATAN-600 are discussed. ...

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• http://www.sao.ru/cats/~satr/RFSymp/abs/11_Golubchina.ps
• A 10-GHz Radio Continuum Survey
• Group IAG

... Director of the RAS ISR . RAS Academician . ... Astrophysics module Kvant of the orbital complex Mir launched in 1987 contains the largest on the station complex of the scientific equipment named the orbital observatory Roentgen. Observatory Roentgen consists of 4 X-ray telescopes, jointly exceeding the range of energies from 2 to 800 keV. ... Among the most significant results that were received in the observatory Roentgen are: . ... measurement of the periods of 9 X-ray pulsars; . ...

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Instruments and Methods 125 Long time tracking of the Sun with RATAN-600 in Radio Schmidt mode V.B. Khaikin, E.K. Ma jorova, I.G. E mov, O.A. Victorov, V.M. Bogod, and S.Kh. ... Cosmic source tracking with unmovable main mirror in a form of cylinder requires a special secondary mirror of double curvature 12 m size or a phased array in the focal plane of an ordinary secondary mirror Ka jdanovskij, 1980. ... Fig. 4 shows the Sun tracking with new drive in speed control mode starting from meridian. ...

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• ASTROMETRIA

The wave complex KEM-3 is designed to measure the parameters of electromagnetic waves in the VLF and ULF ranges. ... The electric antenna is a 1.6 m long dipole made up by two spherical carbon EDS detectors each with a preamplifier. ... The same detector is also used for the VLF device. ... 1. component Ex: 0.1 Hz - 400 kHz; 5*10E(-8)HzE(-1/2) (2 kHz). 2. component Bx: 1.0 kHz - 50 kHz; 10E(-5) nT*HzE(-1/2) (2 kHz). 3. components Bx,y,z: 1.0 Hz - 2 kHz; 3*10E(-5) nT*HzE(-1/2) (100 Hz). ...

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• Radiometric Complex Traverse
• Plasma-wave complex (PWC)

... The well-known spherical aberration in the OTA primary mirror causes most of the light for stellar targets to fall in a large halo (Figs. 2 and 3). The PSF core has nearly the correct diameter, but contains only about 15%of the light. ... The variations with field position are a large effect for WFPC images (Fig. ... This ``breathing'' of the OTA has a noticeable effect on the PSF wings for WFPC data; the wings expand and contract on a timescale comparable to the orbit period. ...

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• Polarization Observations
• The Large Magellanic Cloud's Largest Molecular Cloud Complex: Spitzer Analysis
• HST Focus Monitoring

Static Fourier spectrometers are often used for spectral measurements of the ionosphere emissions. There are two main advantages of Fourier spectrometers (FS) - large geometric factor and high spectral resolution; these parameters are two orders better than for grating spectral instruments. ... In scanning Fourier spectrometer optical and electric modulation of signal is used to avoid this problem, for static Fourier spectrometer there are no such ways. ...

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• Researches of Astronomy and Space Physics Department

A search for biomolecules in Sgr B2, and the massive star-forming region NGC 3576 Paul Jones (ATNF), Maria Hunt (UNSW) etc Biomolecules project ! ... We have looked at 2 positions * Sgr B2 (N) LMH = Large Molecule Heimat, which is where the largest number of large, complex molecules have been detected, a dense, dusty region * IRAS 16562-3959 = G345.5+1.5 - a region found to be rich in simpler molecules, comparable to Orion KL, from Mopra and SEST observations. ... ATCA results at 3 mm (C1077) ! ...

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• http://www.atnf.csiro.au/whats_on/workshops/mm_science2002/talks/thill.pdf
• http://www.atnf.csiro.au/lists/vlbiobs/att-0580/TidAllocation.pdf
• casacore: casa::MSMainEnums Class Reference

... Observations of Pre-biotic Complex Organic Molecules in the Pristine Jet-disk Systems Associated with Sun-like Protostars - DD74/2015 . ...

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• Ranger to the Moon (1964 - 1965)
• TRASP 2
• Virgo Group - Gravitational Wave basics

RTT150 . Russian-Turkish 1.5-m Telescope . ... Telescope has two main foci (Cassegrain and Coude ) and allows to use six optical systems based on Ritchey-Chretien system with a common main mirror . At present scientific observations are being performed at the Cassegrain focus in main optical scheme with focal ratio of 1:7.7. ... flat . ... To use the Coude focus the removable flat diagonal mirror is also needed in the crossing point of declination axis and main optical axis of telescope. ...

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... Secondary Baffle . ... The outside diameter of the tip of ring 5 (the secondary baffle tip) was 1285.7 mm with a range of 0.8 mm p-v. The specifications were 1284.6 and 7.6 mm respectively. ... The outside diameter of the base of ring 5 was 1273.4 mm with a range of 2.0 mm p-v. The specifications were 1272.1 and 8.1 mm respectively. ... The inside diameter of the tip of ring 19 (the primary baffle tip) was 857.7 mm with a range of 0.8 mm p-v. The specifications were 858.0 and 8.6 mm respectively. ...

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• Measurements of 3.5-m Secondary Mirror Motions
• Scale adjustment
• Mirror baffle inspection

... Solar Space Experiments in LPI . ... 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 EUV Coronagraph (SEC), based on the Ritchey-Chretien scheme, to observe the inner and outer solar corona from 0.2 to 4 solar radii in spectral band 290-320 A . ... 2 arc. sec./pix . ... Backside-CCD 2048*2048 pix...

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• TESIS - Telescopes for EUV Spectral Imaging of the Sun

... Astrophysics Group . ... VSA . ... CAT . ... The Very Small Array is a custom-built radio telescope (operating between 26-36 GHz), designed expressly to make high resolution observations of the cosmic microwave background (CMB) radiation on angular scales around and below one degree. ... The VSA has been operated in ?compact array? and ?extended array? configurations (see the technical description below) and data collected to achieve high sensitivity in both regimes have been analysed. ... 1.75 GHz)...

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• G263.9-3.3
• High-frequency Radio Continuum Observations of Giant Radio Galaxies
• VLBI observations of the quasar 3C380

. Description . How SCA-1 measurements are organized. List of publications. Interball Observations of the Dayside Magnetopause. Observations of the Fine Structure of Ion Distribution Function at the Bow Shock. Latest news. Back to the Interball Home Page . Last updated: 17 Feb 1997

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• FM-3I Instrument
• Enhanced aurora [Oulu]

Supernova 2007sr in NGC 4038 . This page is devoted to information on Supernova 2007sr in NGC 4038 . ... Discovered by Catalina Sky Survey (USA). This one turned out to be the brightest northern hemisphere visible supernova of the year 2007. ... Icon generated from the discovery image. This supernova is in the Constellation Corvus . ... Catalina Sky Survey 's discovery page . ... SNWeb has a 2007sr page . ... Confirmation, mirror , mirror . ... JM Llapasset . ... 2008/01/06.208 . ...

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Astronotes Armagh Planetarium's Stellar Blog! ... Our Galaxy . ... Other Galaxies . ... Space Flight . ... When Galaxies Collide (Image credit: ALMA (ESO/NAOJ/NRAO). Visible light image: the NASA/ESA Hubble Space Telescope) . In the southern sky constellation of Corvus (the Crow), we see the Antennae Galaxies (alias NGC 4038 and 4039). ... Your email address will not be published. ... Here you will find the latest news and views from the fascinating worlds of astronomy and space exploration. ...

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... Radio astronomical tests of the engineering model of the space radio telescope (SRT) were completed in Pushchino - see Results . ... Monitoring of the development of the upgrade on-board 1.35-cm receiver (R-SRT-1.35 cm): . ... EM Engineering Model . ... OHCFS-SRT Space Radio Telescope On-board Heterodyne and Clock Frequency Synthesizer set . OHFS-SRT Space Radio Telescope On-board Hydrogen Frequency Standard . ORFS-SRT Space Radio Telescope On-board Rubidium Frequency Standard . ...

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• Navigation Post-Observation Products
• Description of the RadioAstron project, english version
• MILLIMETRON

... Gallery . ... Demolition of the workshop complex . Sidebar Left . Sidebar Top . No Sidebar . Sidebar Bottom . Sidebar Right . Title: Demolition of the workshop complex . Description: The Mechanical, Optical and Electronic workshops were totally destroyed in the firestorm. ... Demolition and cleanup were done by Delta Group. ... Views: 2047 . ... Views: 2715 . ... Views: 1968 . ... Views: 1868 . ... Views: 1836 . ... Views: 1876 . ... Views: 1947 . ... Views: 1833 . ...

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• ANU - Research School of Astronomy and Astrophysics - 5th Stromlo Symposium
• Siding Spring Observatory 2.3 m (looking up at the secondary mirror)

Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Phase range for plots: -0.5 to 1.0 0.0 to 2.0 0.0 to 1.0 . ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... Two period search methods are currently implemented. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . ...

20. APOD: 2008 March 27 - The N44 Complex