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• Космические полеты
• 'Soyuz-TMA' integrated IDS and RS ISS integrated console of manual control loop

Feed cabin Nr. ... Fig. ... This allows to realize the sensitivity at frequency ranges 4.8, 11.2 and 30.0 GHz of 5, 7 and 12 mK by double beam switching mode and by the integration time of the output filter 1s. Input waveguide paths were very long and had big losses. ... The focal line of the feed cabin Nr. ... Data Acquisition and Control System . The Data acquisition system of the feed cabin Nr 2 is based on the new measurement ER-DAS system (Embedded Radiometric Data Acquisition System). ...

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• Observational data
• A Method of Integrating
• Laboratory of spectroscopy and photometry of extragalactic objects :

Microsymposium 38, MS080, 2003 (A4 format) PHYSICAL AND MINERALOGY CHARACTERISTICS OF THE LUNAR REGOLITH IN THE AREAS OF THE THERMAL ANOMALIES. ... Comparison of the local cumulative number of particles N per 104 m2 and photometric roughness parameter I. In this report we research data of the IR thermal radiation, the rough structure of the lunar regolith and mineralogy characteristics upper layer of the surface. ... The spatial graphical function of the lunar-surface thermal radiation. ... Figure 3. ...

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• http://selena.sai.msu.ru/Pug/Publications/Pugacheva%20LPS%2041.pdf
• http://selena.sai.msu.ru/Pug/Publications/ms42/m42_60.pdf

. annotation of talk . V.M.Malofeev, O.I.Malov (PRAO) . Detection of radioemission from Anomalous X-ray pulsar 1E2259+58 . We report on the discovery of pulsed radio emission with period 6.98 s from the first anomalous X-ray pulsar (AXP) 1E2259+586. The observations were made with the LPA FIAN in Pushchino at 111 MHz. The flux density about 70 mJy and the width of integrated pulse is close apon 120 ms. The dispersion measure is about 80 pc/cm 3 that gives the distance to pulsar 3.6 kpc.

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• Gravitational waves from supernova explosions

I will present here some of the work that I, my group and collaborators have done on understanding the heating and cooling of the nearest L* galaxy to our own, Andromeda. Its proximity means that we gain a high resolution picture of a typical galaxy unobtainable anywhere else except for the Milky Way, but being external, we can see the integrated picture at the same time, making comparisons with more distant surveys much easier. ...

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• http://www.mso.anu.edu.au/~geoff/HEA/Magnitudes.pdf
• http://www.mso.anu.edu.au/gsaoi/gallery/rsaa/pics/brochure.pdf
• http://www.mso.anu.edu.au/pfrancis/ObsTech/BrightnessUnits.pdf

... NASA Integrated Services Network (NISN) . ... The NASA Integrated Services Network's mission is to provide a computer communications network designed to support NASA Science flight mission, discipline research programs, and collaborating scientists' affiliate research institutes. ... Use of the NASA Integrated Services Network to support NASA research, related training, and associated technical activities at non-profit institutions of research and education is acceptable. ...

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PENTICTON SOLAR RADIO FLUX VALUES (from SGD Explanation of Data Reports) Daily Solar Flux Values - Penticton -- Daily measurements of the integrated emission from the solar disc at 2800MHz (10.7cm wavelength) have been made by the National Research Council of Canada since 1947. ... The data are tabulated in two forms: the "observed flux" (S), and the "adjusted flux" (Sa). ... The "observed flux" values are useful in ionospheric physics and other terrestrial consequences of solar activity. ...

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Introduction This catalogue contains mainly the atomic data needed in the astrophysical investigations of low-density plasma. It is a revised and extended version of the "Catalogue of Atomic Data for the Rarefied Astrophysical Plasma" (Golovatyj et al. ... Low-density plasma. ... In the present study we represent only the atomic data for computation of sp ectra of low-density astrophysical plasma (most known kinds of it are gaseous nebulae), their thermal and ionization structure. ...

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Multi-Frequency Synthesis in K-band . The Multi-Frequency Synthesis (MFS) permits to realize a good quality imaging of the continuum radio sources in short time. ... The RadioAstron mission will operate one K-band circular polarized channel at fixed frequency 22,232 GHz. ... In general one K-band RadioAstron channel with fixed frequency will be unchanging and compatible with all the ground radio telescopes. ... Progress of the RadioAstron Project in Pictures . ...

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• ОТЧЕТ

... SteMaGE is a research program aimed at improving the way we measure stellar mass in galaxies, map its distribution and understand how it affects galaxy evolution. ... At each position in a galaxy the stellar mass density is computed by comparing the observed optical/NIR emission with a library of models that reproduce different SFHs and dust attenuation. ... This new standard will be used to estimate the local SMF, providing a new unbiased reference for galaxy evolution models. ...

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• Fasti Web Site
• GIANO opens a new window on stellar and planetary astrophysics
• Determination of the Detector Parameters

INFRARED FOURIER-SPECTROMETER SICH-F . ... Instrument work regimes: 1) Inside. 2) Calibration at inside standard sources 2 - 4 times per a rotation. 3) Calibration at "free space" 2 - 4 times per a rotation. 4) Infrared radiation measuring 10 - 40 min. per a rotation. ... Spectrometer consists of the photodetector block and the block of signal processing and control. ... Diagnostic information and attach data will transfer by state telemetric channels. ... Detector temperature. ...

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• Laboratory static Fourier-spectrometer
• Introduction to Plasma Physics

... Measure spectrographic field distortion . ... Test collimation . ... The systems that comprise the 2.5-m Sloan Digital Sky Survey (SDSS) telescope must be tested as installation and integration occurs so that problems are discovered at the component and subsystem level rather than at the system level where debugging is more expensive and time consuming. ... This document complements the telescope tests dependency chart that is available as a postscript file. ... Z1 == azimuth axis (zenith direction)...

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• Telescope Tracking Smoothness
• TUI:Scripts:Built In Scripts:Telescope:Pointing Data
• Figure 3

... At high latitudes, the E-region auroral electrojets and field-aligned currents produce 'radar aurora' that are somewhat more complicated than the equatorial radar echoes. ... Type 4 echoes are a special type of two-stream events associated with anomalous electron heating by the auroral electrojet waves. ... Res. ... Hedberg, and J. A. Nordling, Observations of auroral E-region plasma waves and electron heating with EISCAT and a VHF radar interferometer, J. atmos. terr. ... Observations, J. Geophys. ...

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• Drift mechanisms [Oulu]
• THE LOW ENERGY PLASMA COMPOSITION EXPERIMENT AMEI-2
• Space Weather Dials Interpretation Guide

... News . ... Research areas . ... English News . ... In the spring of this year the scientists of Samara State Aerospace University (SSAU) will proceed to integrated exploration environment in the near-Earth space and its impact on the engineered materials of spacecraft. ... This spring it will be launched into space by the first carrier rocket from the new Russian space launcher complex Vostochniy. ... The equipment set is designed and manufactured in SSAU Institute of Space Device Engineering (ISDE)...

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• Свистула Марина Геннадьевна. Публикации
• StrAU
• Подклетнова Светлана Владимировна. Публикации

. Last updated Aug 3, 1998 by K.Borozdin, kbor@hea.iki.rssi.ru

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• IKI test facilities
• SODART X-ray telescope
• RTT150 telescope: GRB 060526

... Figure 10: Mean power spectrum obtained by time-averagi ng the energy map at each duration. For non-periodic signals, the mean wavelet spectrum is similar to the Fourier spectrum. ... The compromise we reached in allowing for single bump localization (something Fourier cannot do) reduces the spectral accuracy. ... Denote by the Fourier transform of the signal, the Fourier transform of the Mexican hat wavelet. ... by which the wavelet transform is a band-pass filtered Fourier Transform. ...

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• HTML Design Notebook
• Undergraduate Teaching
• Thomson's method of spectral estimation

... Galaxies 99 Cosmic background with model of cloudy interstellar medium Yu. ... Figure 1: Averaged spectrum of the cosmic background I f in frequency range 0.25 200 MHz for the Galactic poles. ... First interpretation of the cosmic noise background spectrum at broad band frequency range 0.25 200 MHz with a model of the cloudy interstellar medium ISM is presented here. ... Synthesized background spectra I f for regions of the Galactic poles at the frequency range 0.25 200 MHz is presented in Fig. ...

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• http://www.gao.spb.ru/english/publ-s/viii-rfs/p129.pdf
• ASTROMETRIA

... T emperature dependence of surface impedance of Tl 2 Ba 2 CaCuO 8- d and YBa 2 Cu 3 O 6.95 single crystals measured in the microwave band. Abstract: . The real part R s and the imaginary part X s of the surface impedance Z s =R s +iX s of Tl 2 Ba 2 CaCuO 8- d and YBa 2 Cu 3 O 6.95 single crystals have been measured with high precision at frequency w/2p= 9.4 GHz in the temperature range 0< T< 140 K. In the Tl 2 Ba 2 CaCuO 8- d . ... A formula describing the curve of . ...

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• Phys. Rev. Lett. 72, 3092 (1994): Neminsky et al. - Temperature dependence of
• Nefyodov Yu.A. - Publications

... AMPLE (Adaptable Minor Planet Ephemerides) is integrated software package to deal with a number of problems concerning minor planets with the aid of IBM-type personal computer. ... compiling a list of all numbered minor planets which can be seen at certain moment within specified sky region and visualization of their mutual positions; . ... As AMPLE is able to reproduce virtually any table of "the Ephemerides of Minor Planets" , it may be considered as computer version of the EMP. ...

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• (Untitled)
• Keywords_32
• Keywords_54

... According to the most popular cosmological paradigm, the greater part of the galaxy mass is accumulated in the dark matter halo. ... The polar ring galaxies (PRGs) reveal external rings or disks of gas, dust and stars rotating in a plane roughly perpendicular to the disk of the central galaxy. ... The shape of the dark halo in the model was chosen so as to achieve the best fit to the observed rotation of both galaxies themselves and their polar rings. ... The SPRC-7 galaxy. ...

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• Solar system sector, archive 1996
• New data on the cpmplex field structure of chemically peculiar stars
• topic_en