... Лекция 1 (33K) | Лекция 2 (25K) | Лекция 3 (23K) | Лекция 4 (30K) . Лекция 5 (26K) | ... Лекция 7 (24K) | Лекция 8 (32K) . ... Лекция 10 (22K) | ... Лекция 12 (20K) ] . ... Это спецкурс по теории линейных операторов в гильбертовом пространстве H (и шкалах гильбертовых пространств). ... это неограниченный оператор, имеющий непустое резольвентное множество \rho(A) на комплексной плоскости и компактную резольвенту R_A(\lambda)=(A-\lambda I)^{-1} при \lambda\in\rho(A). ...

SPECTRUM ANALYZER OF MAGNETIC PHENOMENA SAMW . Spectrum analyzer allows onboard computation of electromagnetic waves spectra registered (observed) in the ionosphere and magnetosphere in the ELF/VLF frequency band. ... It consists of magnetic antenna, preamplifier, 16 bit sigma delta AD converter, DSP processor and telemetry interface. ... The channels of lower frequencies are averaged and transmitted with lower repetition rate so the telemetry volume is reduced. ... Dynamic range: 90 dB . ...

. 6553 - 6575 A . 6575 - 6593 A . 6593 - 6609 A . 6609 - 6634 A . 6634 - 6644 A . 6644 - 6663 A . 6663 - 6678 A . 6678 - 6705 A . 6705 - 6727 A . 6750 - 6753 A . 6753 - 6772 A . 6782 - 6807 A . 6804 - 6829 A . 6820 - 6844 A . CCD-1300LN Spectral sensitivity . Head of homepage . Data archive .

... RC0015+0503a . RC0015+0503b . RC0015+0501 . ... Radio source parameters . ... R.A.(B1950) Dec.( ... MHz] size["] flux[mJy] 00:12:48.50 +04:44:53.3 1425.0 10.0x4.6 75 00:12:48.90 +04:44:37.7 7.6x4.6 16 R.A.(J2000) Dec.( J2000) LAS Sp. Morphol. ["] index 00:15:22.62 +05:01:33.6 16.3 1.03 D,FRII 00:15:23.02 +05:01:18.0 ---------------------------------------------- # R.A.(J2000) Dec.( ... R.A.(J2000) Dec.( J2000) R.A.(B1950) Dec.( ... Last updated 11 Dec 2000 . ...

Next: Imaging Polarimetry with NICMOS Up: NICMOS Data Calibration and Previous: The Photometric Performance of . ... NICMOSlook and Calnic C . ... Extracting spectra from a large number of NICMOS grism images requires a convenient interactive tool which allows a user to manipulate direct/grism image pairs. ... NICMOSlook and Calnic-C are two programs that were designed to take advantage of the fact that the NICMOS grism mode typically consists of taking both a direct and a grism image. ...

Спектр (от лат. spectrum - представление, образ, видение) . ... Спектром электромагнитного излучения называется совокупность всех значений его интенсивностей для любых длин волн, частот или энергий его квантов . ... Непрерывный спектр электромагнитного излучения в оптическом диапазоне представляет собой сплошную непрерывную цветную полоску с изменением цветов от красного до фиолетового. ... Другими слова ми, если в потоке излучения присутствуют волны любой длины, оно имеет непрерывный спектр. ...

... Another option is to buy slides of astronomical objects at different wavelengths to show students why astronomers use different bands of the spectrum to bring out specific characteristics in celestial objects. ... He then uses the camera to scan the entire classroom, asking students to identify what they are seeing. ... Once students see light in action, they can investigate its properties - such as frequency, wavelength, and interference - with wave experiments. ...

... Before the modern era of technological astronomy, to know anything about the Universe beyond our planet we relied on light. ... Historically the two rival ideas were that light was either a stream of tiny bullet-like particles or a wave wobbling its way through space. ... The light we see (visible light which is not the tautology it sounds) is only part of the electromagnetic spectrum, a great sweep of radiations which also includes radio, infra-red, ultra-violet, x-rays and gamma rays. ...

... Tonight's Sky . ... Venus . ... Astronomy for Kids . ... Venus Climate Orbiter Akatsuki inserted into Venusт?? orbit . After missing on their first attempt in 2010, the Japan Aerospace Exploration Agency successfully inserted the Venus Climate Orbiter Akatsuki into orbit around Venus. ... The Japan Aerospace Exploration Agency (JAXA) successfully inserted the Venus Climate Orbiter Akatsuki into orbit around Venus. ... Only registered members of Astronomy.com are allowed to comment on this article. ...

Stellarium 0.12.3 . ... Classes . ... StelSphericalIndexMultiRes Class Reference . ... voidљ . ... Insert the given object in the StelSphericalIndexMultiRes . ... template<class FuncObject > . ... processIntersectingRegions (const SphericalRegionP &region, FuncObject &func) const . ... processAll (FuncObject &func) const . ... processBoundingCapIntersectingRegions (const SphericalCap &cap, FuncObject &func) const . ... processContainedRegions (const SphericalRegionP &region, FuncObject &func) const . ...

... Spectrum-RG is joint project of Russian Federal Space Agency (Roscosmos) and German Space Agency (DLR) of X-ray astrophysical observatory. Its main aim is to make all-sky survey in the X-ray (0.5-11 keV) band in order to find all massive clusters of galaxies in the Universe, millions of active galactic nuclei, including obscured ones and hundreds of thousands of Galactic X-ray sources. ... eRosita (Germany) X-ray grazing-incident mirror telescope, consisting of 432 mirrors combined in 7 modules. ...

APO/GIFS Instrument Factsheet The Goddard imager and Integral Field Spectrograph (GIFS) has recently been commissioned on the APO 3.5 m telescope. This factsheet presents a high level overview of the GIFS instrument. ... GIFS Imaging The GIFS imaging mode is used for imaging science and target acquisition for the IFS mode. ... Imaging Mode pixel scale: 0.168"/pixel · Comparison to Other APO 3.5m instruments: The GIFS field of view is smaller than SPICAM, but the filter set is far more extensive. ...

... 400mm f/2.8 Nikor lens: images the sky on the entrance slit. ... The optical system maintains image quality along the slit length so that each row of the image is a spectrum of that spatially selected region of the sky. 180mm f/2.8 Nikor lens: collimates the light from the slit. ... The auxiliary optical platform on WISPI now accomodates a short focal lens and a guiding/imaging video system that may use sub-pixel corrections to provide feedback to the tracking drive motors. ...

Trace: q3c . start : q3c . ... SAI VO Projects . ... Help on Wiki search . ... dropdb q3ctest createdb q3ctest psql q3ctest /usr/local/pgsql/share/contrib/ q3c .sql psql q3ctest /usr/local/pgsql/share/contrib/pg_sphere.sql \timing on DROP TABLE running_ q3c ; DROP TABLE running_pgsphere; CREATE TABLE running_ q3c (id INT, ra FLOAT, dec FLOAT); CREATE INDEX running_ q3c _idx ON running_ q3c ( q3c _ang2ipix(ra, dec)); CREATE ... SAI VO | ... SAI MSU | ...

User has a possibility to add new string (row) with observed data to the table, to insert string between existing ones, to edit observed data or to delete some strings. To add string select task item in menu bar ( O – C , Identification, Plates, or Observatories ) and then Add String in drop-down menu. ... Marked strings will disappear. ... To select a place for inserting just mark some string, select Paste item in drop-down menu, and block copy appears above this string. ...

... 1999: . A new fiber multiobject spectrograph of the prime focus of the BTA was manufactured, designed for the spectroscopy of low and moderate spectral resolution of up to 70 objects at once, visible in the telescope's field of view sized 12'. ... The new spectrograph brought an opportunity to explore the objects with absolute magnitudes m=22-23 in the R-band. In 1999 the spectrograph was used for the BTA observations within two programs. ... Archive . ...

... This file table3 82 660 Observed wavelengths, laboratory values and identifications -------------------------------------------------------------------------------- Byte-by-byte Description ... Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- SpOrd Spectrum order 5- 12 F8.3 0.1nm SolLam Wavelength determination of all solar and telluric lines measurable on the ... Note (6): J: Junkes et al., ...

... Search . ... Astrophysics Group . ... NP-CAMB . ... We provide a set of routines for producing CMB power spectra with a variety of primordial power spectrum models based on the paper astro-ph/1203.1252 . We provide a model independent node based reconstruction using either linear or cubic spline interpolation with codes to integrate with CAMB and CosmoMC . ... We will shortly provide a set of routines for the generation of spectra using the Lasenby & Doran Closed Universe Model astro-ph/0307311 . ...

... 44, No. 3, 2002, pp. ... WORKSHOP FULLERENES AND ATOMIC CLUSTERS (St. Petersburg, Russia, July 2­6, 2001) Phase Transitions in Hydrofullerene C60H36 Studied by Luminescence and Raman Spectroscopy at Pressures up to 12 GPa1 K. P. Meletov* , **, S. Assimopoulos*, G. A. Kourouklis*, and I. O. Bashkin** * Physics ... Solid State Physics, Russian Academy of Sciences, Chernogolovka, Moscow oblast, 142432 Russia Abstract--The effect of hydrostatic pressure on the photoluminescence and ...

The Star called the Sun. The Sun as the star . ... The visible star value . ... Spectrum class . ... 149 597 870 km . ... The Solar energy sourse is the core transformation of the Sun, where temperature is 15 000 000 K. The energy from inside is carried by irradiation and then in the external layer with 0,2 Ra of thikness - by convection. ... The Earth, situating far from the Sun (149 mil km), receives about 2.1017 W of the Solar beam energy (see item "The Solar constant" ). ...