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Back . Moveable feed-cabine #1 with secondary mirror (9*5.5m) is equiped by six continuum radiometers complex in wavelenths range 1.38 - 31 cm. Near 70% of time it used with antenna "Northern Sector".

Emission Line Diagnostics in a ``No UV Bump'' Quasar PHL909 Smita Mathur, Belinda Wilkes, Martin Elvis and Jonathan McDowell Abstract PHL909 is a quasar with unusually low ultraviolet luminosity (blue bump strength C UV=IR = \Gamma0:20 compared to an average value of 0:4 (McDowell et al. ... The intrinsic continuum of PHL909 ( i.e. as seen by the BELR ) may thus be similar to the `standard' continuum, with a big blue bump, reddened along the line of sight. ...

Next: NOVIDAS and UVPROC II-Data Archive and Reduction System for Nobeyama Millimeter Array . ... The RATAN-600 radio telescope allows us to carry out simultaneous multi-frequency observations using wide-band radiometers. ... Using these features a flexible astronomical data processing system (FADPS), operating on different UNIX platforms, was created. ... FADPS commands may be executed directly in UNIX, in scripts, or using a special shell for our data processing system in the X-Window system. ...

PRO normalise, creg , cforder ;; convert flux spectra to normalized spectra ; COMMON fileblock COMMON fitsblock COMMON procblock COMMON colorblock ;; Input ; ; creg = [w1l, wlu, w2l, w2u, ....] ; pairs of wavelength defining regions for fitting the continuum IF ( n_params() LE 1 ) THEN cforder = 3 ;; assumed order for continuum polynomial print, cforder ;; evaluate the median spectrum specm =fltarr(nwave) FOR iw=0,nwave-1 DO ...

... Fundamental core Alfven mode ~20Hz Fundamental crust shear mode ~10 ­ 40 Hz Strong coupling leads to non-trivial dynamics. ... Initial crustal displacements decay in <second What happens then? crust · Global modes are strongly damped when inside Alfven continuum (L.06,07, Gruzinov 08) · cf. ... Crustal modes Alfven continuum (edge and gap modes) Tangling: effective shear modulus, discrete modes' grid Mass loading in the core (superfluidity, proton fraction) Transient QPOs Successes: 1. ...

... Executive scientist on object Ratan-600, Academician of RAS Parijski Y.N. Deputy director of SAO RAS on radiotelescope Ratan-600 Mingaliev M.G. Radio astronomy department . Radio astrophysics laboratory . Group for study of galaxies and cosmology . ... Laboratory of continuum radiometers . ... Group of continuum observations . Group of the Sun study . ... Laboratory of the Sun study . ... Feed cabin N1 . ... Schedule archive (Russian) . ... Observation data archive of RATAN-600 . ...

Астроплощадка: 53 20 56,505 N 83 46 07,735 E, H абс. = 209 м. + Информационные каналы . ... Анк а дня . ... Статьи . ... Солнце ? ... Картинка дня . ... Мониторинг Солнца . Вид Солнца сейчас . Новые статьи . ... Т Тельца и переменная туманность Хинда . ... MWC 922: красная квадратная туманность . ... Copyright 2002-2014 . ...

... Obs., vol.36, December, 2000, p.64-68. ... Solar Physics, 2000, 195, 401-420. ... A.M. Uralov, H. Nakajima, V.G. Zandanov, and V.V. Grechnev Current sheet associated radio sources and development of the magnetosphere of active region revealed from 17 GHz (NoRH) and Yohkoh/SXT data // Sol.Physics, 2000, 197(2), 275-312. ... Russian-Chinese Workshop 'Solar-Terrestrial physics and its applications (Space weather), Abstracts, 14-19 December 2000, Irkutsk, 2000, p.5 . ... V.G. Ledenev. ... 2000. ...

. B0101ћ8-3012 . Redshift = 0.89, Separation = 16 arcsec. Projected separation is 71/h kpc. The difference in the measured velocities is 300?850 km/s. From the flux ratios, it is clear that the continuum shapes are also remarkably similar. | Front page | . | << - QSO close pairs | . Robert J. Smith, ">rsmith@mso.anu.edu.au Last modified: Fri Sep 24 11:39:02 EST 1999 .

... There are preliminary series of photometric and radio spectral observations of the above-mentioned stars, archival data on the light curves of the stars, results of the search for OH and H 2 O maser emission in IRAS point sources that possess the IR parameters similar to Miras. ... The aim is a detailed study of the maser emission variability. ... In 1996-1997, astronomical observations of Mira Ceti-type stars (miras) were carried out in three spectral ranges: optical, infrared, and radio. ...

pro save_event,event COMMON all,draw1,draw2,cont1,cont2,savename widget_control ,event.id,get_ uvalue = uvalue case uvalue of 'OK1': begin widget_control ,draw1, get_value =val1 wset,val1 x=tvrd() widget_control ,savename, get_value =name write_gif,name(0),x widget_control ,event.top,/destroy end 'OK2': begin widget_control ,draw2, get_value =val2 wset,val2 x=tvrd() ...

... 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....

Elsevier Ed itorial System(tm) for JASR 2006 Manuscript Draft Manuscript Number: Title: Determination of K, Ar, Cl, S, Si and Al flare abundances from RESIK soft X-ray spectra Article Type: Contributed Paper Section/Category: E2.4 - Solar Magnetic Field and Activities Keywords: solar physics; X-ray flares ; spectroscopy; abundances Corresponding Author: Dr. J. Sylwester , Corresponding Author's Institution: Space Research Center First Author: J ... All flares were observed early Fig. ...

... 9) Oknyanskij V.L. 1994, "Optical-radio time delays in Q0957+561", Odessa Astronomical Publ., ... 11) Oknyanskij V.L. 1994, "Connection between X-ray and optical variability in NGC4151", in Proceedings of Int. Conf. ... 1994. 12) Oknyanskij V.L. 1994, "Connection between X-ray and optical variability in NGC4151", Astrophys. and Space Science, 222, p.157. ... 14) Oknyanskij V.L., van Groningen E., 1997, "Optical spectral variability of NGC4151 in 1990", Astronomical and Astrophys. ...

University Satellites and . Space Science Education . ... Abstract Submission List of submitted abstracts . ... The abstract you have submited . The 19th century observation of light phenomena versus space-time continuum. ... The author show endeavours for adjustments of optical phenomena and electrodynamics processes with the 19th century concept of ether. ... Skobeltsyn Institute of Nuclear Physics, Moscow State University, 2005-2006 . ...

Microsymposium 40, abstract 88, 2004 (A4 format) GAMMA RAYS FROM MAJOR ELEMENTS BY THERMAL NEUTRON CAPTURE REACTIONS: EXPERIMENT AND SIMULATION FOR PLANETARY GAMMA-RAY SPECTROSCOPY. ... Then the calculation can be restarted by producing gamma rays and let them trans- GAMMA RAYS FROM MAJOR ELEMENTS BY THERMAL NEUTRON CAPTURE REACTIONS: N. Yamashita et al. port and react, with initial energies determined the outside multiplication and initial locations wh neutron capture reaction took place. ...

... Aims: Today, large ground-based instruments, like VISIR on the VLT, providing diffraction-limited (about 0.3 arcsec) images in the mid-infrared where strong PAH features appear enable us to see the flaring structure of the disks around Herbig Ae stars. Although great progress has been made in modelling the disk with radiative transfer models able to reproduce the spectral energy distribution (SED) of Herbig Ae stars, the constraints brought by images have not been yet fully exploited. ...

Юпитер - грозный гигант . ... Исследование Солнечной Системы - Юпитер . ... Юпитер . ... Строение Юпитера . ... Полярный вихрь . ... Резкий перепад температур, по сравнению с окружающими воздушными массами, создают восточные ветра, которые сохраняют полярную атмосферу, включая стратосферную дымку, изолируя их от остальной атмосферы. ... Так как у Юпитера самая большая магнитосфера во всей Солнечной системе, то эффект от влияния солнечного ветра должен быть значительным в пример другим планетам. ...

INNER POLAR RINGS REGULAR LENTICULAR GALAXIES 1 K. Sil'chenko 2 Sternberg Astronomical Institute, 119992 Moscow, Russia; Isaac Newton Institute Chile, Moscow Branch; olga@sai.msu.su Afanasiev Special Astrophysical Observatory, 369167 Nizhnij Arkhyz, Russia; vafan@sao.ru Received 2003 December accepted February 4 ABSTRACT have investigated a sample of galaxies, mostly with circumnuclear dust lanes orthogonal their major axes, chosen from Hubble Space Telescope Wide Field Planetary Camera 2 images. ...