RTT150 . ... HEAD IKI . This page is a search interface through RTT150 observationsdatabase which is stored at IKI. According to the agreement between participantsof RTT150 project, observational data fully belong to the institution which hascarried out this observation for one year, are available to all three partiesinvolved (IKI, KSU and TUG) during the second year and become freely accessibleto the whole astronomical community starting two years after observation date. ...
... The dependence of velocity ellipsoid parameters for various types stars upon theirage was investigated. ... For metal-rich stars ([Fe/H] -0.1) the shape of velocity ellipsoid becomes more spherical with increasing age of the stellar group and it approaches the equilibrium shape. ... По данным uvby -фотометрии, изохронным возрастам и собственным движениям ~3500 F -звезд диска в окрестности 80 пс от Солнца исследованы зависимости параметров эллипсоидов скоростей различных звезд от возраста. ...
Next: Description of algorithm Up: A Method of Integrating Previous: A Method of Integrating . The fast real-time processing of radiometer signals can be successfully implemented because of the existence of modern high performance ADC and data acquisition systems. ... On the other, hand the median-like rank estimation are very robust to spike type contamination (up to 50%), but there is loss in efficiency in case of normally distributed, spike-free signal. ...
... The HH flow associated with young stellar object HL Tau has an exciting history and even until now the origin of some its features is not clear yet. ... Knotty structures of Herbig-Haro jets are common phenomena and knowing the origin of such structures is essential for understanding the processes of jet formation. ... In the flow detected compact knots with high (-150 km/s) and bow shape structures in front of those, with low radial velocities (-50 km/s). ...
... In 1930, Trumpler noticed that linear diameters (LD) of open clusters increase with distance (D) from the Sun. ... Since that time, the interstellar absorption has become one of the best studied factor in astrophysics, and we may hope that current OCL distance scales are free from this LD-D correlation. To verify if this is the case we have chosen several modern OCL distance scales and test them with the same clusters and the same angular diameters that Trumpler had used back in 1930. ...
Estimating the NEO Population and Impact Risk: Past, Present and Future . ... Since most of the risk resides in the largest impactors, finding that fraction of the largest bodies, and that none of them has a significant chance of impacting in the next century or so, "retires" more than 90 % of the impact risk, including most of the risk of a globally catastrophic impact event. ... In the mid-size range, from ~150 m to ~1 km, the main risk is from tsunami generated by an ocean impact. ...
... CORBA Client/server architecture needs tools to manage communication between the different components. ... A CORBA class is defined by its interface, specifying in the Interface Data Language (IDL), the methods, their parameters and return values to be used on the client side and to be implemented on the server side. ... 214 Wenger and Frisґ ee IDL file (CORBA class description) IDL compilation Client code STUB code SKELETON code CORBA class implementation Server Client server code Figure 1. ...
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Ссылки http://www.adass.org/adass/proceedings/adass00/reprints/O3-04.pdf -- 70.6 Кб -- 29.05.2001 Похожие документы
Электронная библиотека астронома-любителя. ... библиотека . архив RSN . ... Ru.Space.News: . Май 1998 . ... Дата: 14 мая 1998 (1998-05-14) От: Alexander Bondugin Тема: JSC Becomes First ISO 9001 Certified NASA Field Center Привет всем! ... From the mountain's extreme environment, health data will travel from the base camp to the NASA-Yale telemedicine project. ... NASA has been a pioneer in telemedicine since the beginning of human space flight. ...
... The frequency and time resolution connected by the (a) Kotelnikov-Shannon theorem (b) Heisenberg uncertainty principle (c) probability density (d) Euler equation 5. The window (Gabor) transform differs from wavelet-transform because (a) the first one doesn't allow to detect the changes of spectrum in time (b) the first one doesn't allow to reconstruct the function from it's decomposition (c) wavelet-transform is continuous (d) the resolution of wavelet-transform is adapted to the frequency 6. ...
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Ссылки http://lnfm1.sai.msu.ru/grav/english/lecture/filtering/testN1.pdf -- 36.2 Кб -- 24.02.2009 Похожие документы
Date : Fri , 27 Feb 2009 01:19:03 . ... the European Week of Astronomy and Space Science which will be . ... UK).. - the Abstract and Early Registration deadline is 9th March 2009 ; . ... for those wishing to become member of the EAS/RAS and as a result . ... http://www.jenam2009.eu/ . ... Registration now open for the "European Week of Astronomy and Space Science" (JENAM2009) . ... The LOC of the "European Week of Astronomy and Space Science" . ... The "European Week of Astronomy and Space Science" . ...
Maria M. Katsova . I am a Leading Researcher in Stellar Astrophysics Department of SAI MSU . I began to work at Sternberg Astronomical Institute (SAI) in 1967, graduated from Moscow State University (MSU) in 1971, Ph.D.(MSU) since 1984. And now I become a Doctor of Sciences (Full Doctor of the Physical and Mathematical Sciences)(MSU, since 1999). ... I am a member of European Astronomical Society (EAS), Euro-Asian Astronomical Society (EAAS), National Geographic Society (NGS). ...
... Under certain conditions, like those in the nucleus of a QSO, all atoms can be made to emit light at particular wavelengths. ... If that source is approaching the observer, the wave is squashed up onto itself making the wavelength shorter. ... This is redshift. ... You can see how the section of the QSO spectrum which we observe changes with redshift. ... We then see how far we had to slide the observed spectrum along the scale to make it match and that is the objects redshift. ... The 2QZ team . ...
... Objectives of the study . To survey and evaluate the technical and economical feasibility of European initiatives by start-up companies, for privately-funded crew vehicles for commercial human space flight. ... New commercial markets, among them space tourism, have a great potential to become major drivers in space technology development. This study aims at the assessment of the feasibility of European initiatives to address these new markets through the development of crewed space vehicles. ...
. 5.24. Now I am in the Aeroflot plane. I discovered that I had become estranged from Russian people. The Russian personnel looks a bit strange for me.
System of astrometric databases of Pulkovo observatory. ... Pulkovo database of observations of visual double stars . ... The 3rd database contains relative positions of selected double and multiple stars, and stars with possible invisible satellites. The database requires catalog of relative positions of visual double stars, based on photographic observations performed since 1960 on Pulkovo 26-inch refractor, and similar catalog based on CCD observations, obtained since 1995. ...
A Large Programme 171.A-3045 (PI: Cesarsky) has been approved in period 71 to carry out a spectroscopic survey in the CDF-S with VIMOS, now installed on UT3. ... MOS (LR_Blue/MR grisms) . ... The VIMOS coverage of the GOODS field (right). ... With an average integration time of 4h per mask and 30% overheads, this makes a total of 125h. The VIMOS spectroscopic campaign is designed to complement the FORS2 spectroscopic program. ... OII],Hbeta,[OIII],(Halpha),CaII H . ... OII],CaII H CIV,AlIII . ...
What is the VSM ? ... VRML = Virtual Reality Modeling Language. ... One of the best VRML viewers, if not the best, is Netscape Navigator with Live3D plugin. ... Warning: if you use any other viewer, spacecraft will probably look like parrots or clowns because each VRML viewer treats colors in its own unpredictable way. ... You can use these VRML models freely in any way you like, but: 1) let me know you use them; 2) if you add them to your Web page, a reference to the VSM must be there. ...
. Comment on J1842+7946 . Comparing the brightnesses of the two main features seen in our 5 GHz image with higher frequency VLBI images available in the literature (at 8.4 GHz from the USNO database and at 15 GHz by Kellermann et al. (1998)), one can conclude that the NW component has a steeper spectrum since the SE one becomes relatively stronger as the observing frequency increases. VLBApls home page . Last modified: 16 Oct 2000
... Space flight . Crew training . ... The contemporary world opinion, while welcoming the efforts of different states aimed at realization of manned space flights, still considers these efforts insufficient, over-bureaucratized and too slow. ... The more up-to-date is the basic training program for a cosmonaut/astronaut or a manned space flight participant (hereinafter referred to as the student) that is being offered to your interested attention. ... Pre-flight space training (PFST). ...
... Research Innovation . Schools . School of Biology . ... Dean?s Office . Departments . ... Geology Department . ... School of Physics . ... Academician I.M. Lifshyts Theoretical Physics Department . ... Crystal Physics Department . Experimental Physics Department . General Physics Department . ... Low-Temperature Physics Department . ... Solid Body Physics Department . ... Since 1952 Biology research station has become the part of School of biology as the base for field practices. ...