. Composition | Objectives | Capabilities and samples | Request for work | Back to main page . If you have any questions, please contact us: rp@iszf.irk.ru . http://esceir.iszf.irk.ru/lchmen/skhema2en.htm . Last modification: 2.06.01.

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• Functional scheme of SW radiochannel characteristics operative diagnostics
• East Siberian Center of Earth Ionosphere Research. Chirp ionosonde.
• East Siberian Center for the Earth's Ionosphere Research. SW radiosignal

Next: Optical and other high Up: An overview Previous: The magnetic fields of . ... Individual pulses very variable in intensity . Stable profile if several hundred pulses added . Strongly linearly polarised . Monotonic polarisation position angle swing through the pulse implies the origin is near a magnetic pole . Much more complex polarisation characteristic in msps indicating more complex field . ... Thu Dec 19 15:15:11 GMT 1996 ...

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• Characteristics of the MOST Survey
• Determining UV Variables and Their Characteristics
• The spectral characteristics of the 2dFGRS-NVSS galaxies

... Figure 3 shows several tails resulting from trap 2-637. ... The solid line shows a simple exponential decay, as described in our idealized model. It appears that the behavior of the bright traps has been relatively constant with time, and the simple exponential decay provides a fairly good fit to the data. ... What about the dark tails seen just above some of the traps? ... For example, the dark tail decay rate for trap 2-337 is only about 3% while the bright tail decay rate is 19%. ...

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• WFPC and WFPC 2 Instrumental Characteristics
• Summary of new COS Lifetime Position Characteristics
• Biretta: WFPC and WFPC 2 Instrumental Characteristics

. Next: Atmospheres Up: R CORONAE BOREALIS STARS Previous: Numbers and distances . Atmospheres . Pulsations . Frequency of fading events . Anatomy of a decline . Simon Jeffery . 2002-01-25

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• Physical Characteristics
• Atmospheres
• Armagh Observatory

The studying of coherent structures and structural properties of a turbulence are the following: . ... the investigations of nonkolmogorov regimes of strong turbulence both in the usual- and magneto hydrodynamics related to the cases of finite correlation times of fluctuations, the analysis of their characteristics dependence on the external random force strength (together with S.N.Gordienko); . ...

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• MAGION-4 Spacecraft (C2-X)

... Set of 8pcs Hot Cartoon Minion Dave Characteristic 5 to 6cm Collection Figure Model . ... Figure Height: 5~6 cm . ... Animation Models . ... Package Contents: 8 x Figure Model . ...

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• PGADRUMKIT4 - Shure - Shure Set of 10Pcs Anime the Second Generation Funny
• Полусапоги s.Oliver - s.Oliver - s.Oliver Сетевое зарядное устройство Ginzzu

... Solar flare activity is produced by the processes of accumulation and release of energy in an active region. ... In the framework of study of solar active regions, producing powerful flares the researchers from the RATAN-600 radio telescope have detected sources with features in the form of a sharp drop in the intensity of polarized radiation in various parts of the recorded frequency range (2-16GHz), sometimes changing the sign of polarization. ...

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... Одним из главных примеров будет служить (до конца не решенная) задача вычисления полных инвариантов Громова-Виттена проективной прямой. ... У.Фултон, Теория пересечений, М., Мир, 1989 . ... 23 декабря продолжение доклада В.Пржиялковского "О вычислении инвариантов Громова-Виттена полных пересечений" . ... Собственно методы вычисления будут обсуждаться на этот раз. 16 декабря доклад В.Пржиялковского "О вычислении инвариантов Громова-Виттена полных пересечений" . ...

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• Characteristic classes (Fall 2000)
• Characteristic classes and intersection theory (Fall 2010)
• Characteristic classes and intersection theory (spring 2009)

Measuring Profile Characteristics of HI spectra in IDL . Gomathi Thai, with the help of Tapasi Ghosh, has rewritten the old analyz (and uni-pops) routines for measuring the profile characteristics of HI data into IDL. ... First is to average the two polarizations, then apply smoothing (or not), fit and subtract a baseline, and finally calculate the velocity, velocity width, area under the curve using the five options that the MSR program in ANALYZ is currently using. ...

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• ALFA Front End Optics

.

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• CCDs for Material Scientists
• Thermal History of the Universe
• Orbital Properties of the Solar System

... CHARACTERISTICS . FIBER OPTIC PLATES . TAPERED FIBER . ... Fiber Diameter . ... 1.0 . ... 102 . ... YES . ... 180 . ... Corning 7575 . Corning 7576 . ... Sealing Metal . ... Metal . Corning 9008 . ... Tapered Ratio . ... 2: FOP:t=3mm,Wavelength=550nm Tapered Fiber Optics:t=15mm,Wavelength=550nm . ...

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• Group IAG
• HyperLEDA documentation: compilation of Color index (a112)
• Graphic Devices

Astronomy Discussion Forums . ... ONE MORE STATE CHARACTERISTIC OF THE MATTER . ... Post Message | ... 1)So, my conclussion is that the Gravitation mostly is the pressure by the bodies larger by size on the bodies relativly smaller by size, , at expense of bigger extension of the bigger by size bodies in the space. ... arkadiv@012.net.il . ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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... We present a computer program for modelling energy flux distribution and light curves of eclipsing binaries from far ultraviolet to infrared regions. The Roche model is assumed. Proximity effects of components (reflection of radiation and surface gravity darkening) are taken into account. ... Figure 1: The surface temperature distribution for Algol A-B system before (upper plot) and after (lower plot) correction for temperature due to the irradiation effect. ...

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• Modelling Spectro-photometric Characteristics of Nonradially Pulsating Stars
• ADASS 2003 Conference Proceedings

... Q abs (x) . albedo (x) . ... n =1.3, 1.5, 1.7; . ... fig . ... Q abs =0; albedo=1 . ... Dependence on the diffraction parameter rho with variations of refractive index m=n+k i . ... Q ext (rho) . Q sca (rho) . Q abs (rho) . albedo (rho) . g (rho) . ...

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• Database of Optical Properties -- Level: subpage
• Database of Optical Properties -- Level: database
• Introduction

... Note that in the low-mass model, the ``secondary'' is more massive than the visible ``primary''; however, we shall follow the convention used in most of the Aurig? literature and continue to refer to the F star as the primary because it is clearly the primary source of luminosity of the system. Doppler shifts of absorption lines seen during eclipse imply an orbital velocity at the edge of the secondary more compatible with the low-mass model (Saito et al. ...

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• Introduction
• Vertical Structure of the Secondary: Hydrostatic Model

... Mokhovaya st., 11, Moscow, 103907, Russia. ... Proceedings of ECCTD?01 -European Conference on Circuit Theory and Design, . ... An approach to design of chaotic oscillators with preassigned spectral characteristics is proposed and its practical realization is demonstrated. The basic idea of the approach is to form a frequency-selective circuit and to connect it to a harmonic oscillator so as to provide generation of chaotic oscillations with given spectral characteristics. ...

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• Research Activities of InformChaos Lab.
• Project 8 - RFBR - Dynamical and non-equilibrium electron transport and
• Single-transistor microwave chaotic oscillator - NOLTA-2000

... Research objects and scientific purposes . Space scientific program includes development and launch of two supersmall spacecrafts "Universitetskiy" and "Kompas-2" intended for monitoring of radiation conditions near the Earth. ... All the studies conducted in the near-Earth space are characterised by strong radiation fields. ... The circular polar orbits, which cover all the near-Earth space, are the most favorable for comprehensive studies of the radiation conditions near the Earth. ...

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MAIN CHARACTERISTICS BASIC MODIFICATIONS TEST RESULTS . ... SOYUZ TMA . SOYUZ TMA SPACECRAFT . MAIN CHARACTERISTICS . Name of characteristic, dimensions . ... Spacecraft mass, kg . ... Descent module mass, kg . ... during spacecraft docking . ... Geometrical characteristics of the spacecraft, mm . ... 2.6 / 1.4 . ... 3.6 / 2.6 (via Soyuz ТМ) . ... Soyuz FG . Developed for the Soyuz TMA spacecraft, has passed flight testing during the Progress spacecraft launches in the years 2001-2002. ...

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• S.P. Korolev RSC Energia - International Space Station
• RSC "Energia" - Land Launch
• S.P. KOROLEV ROCKET & SPACE CORPORATION ENERGIA

... Visible Distribution of Galaxies. ... Features of Elliptical, Lens-Shaped, Spiral and Irregular Galaxies. Galaxies with Bar. ... Distribution of Surface Brightness of Surface and Spiral Galaxies. ... Color Characteristics of Galaxies. ... Methods of Galaxies' Mass Determination. ... Hidden Mass of Spiral Galaxies. ... Features of Dark Matter Distribution in E and SO Galaxies. ... The Whole Number of Galaxies and Their Density by the Results of Observation on the 'Hubble' Space Telescope. ...

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• Solar Physics
• General Astrophysics
• ENERGOSPECTROMETER OF IONOSPHERIC PLASMA P3-3

... Observations of precipitating (Jp) and trapped (Jt) energetic (> 30 keV) particle fluxes at the ionospheric altitudes within the auroral oval region has revealed the existence of a sharp boundary separating the poleward zone of isotropic precipitation (Jp = Jt) from the equatorward zone of weak loss cone filling (Jp << Jt) at all local times (Sergeev and Malkov, 1988). ... boundaries for higher energy particles are located at lower latitudes than boundaries for lower energy particles . ...

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• Substorm current wedge [Oulu]
• Solar wind and IMF [Oulu]
• Point of Agenda; Jun. 1995 CONPAS workshop