... Left: A POSSM plot of the uncalibrated spectrum of DA 193 at 1.66 GHz on a baseline Bear Lakes to Noto. ... The phase slope as a function of frequency is clear evidence for a small delay error in the correlator model. Right: The same data as shown on the left, but corrected for a delay error and a residual fringe rate. ... Left: A VPLOT plot of the uncalibrated amplitude (upper frame) and uncalibrated phase (lower frame) as a function of time for the source DA 193 on a baseline HartRAO to Noto. ...

NNo GCVS 1950.0 2000.0 Type Max Min Epoch Year Period M-m Spectrum References Other design. \n"; NSV B1950.0 J2000.0 Type Max Min(Ampl.) Ref. Oth.design. Sp. GCVS design.\n"; NSVS 1950.0 2000.0 Type Max Min References Spectrum HD Sp. GCVS design.\n";

... 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 . ...

What if we could determine if a given star is likely to host a planetary system like our own by breaking down its light into a single high-resolution spectrum and analyzing it? ... The dark bands result from specific chemical elements in the star s outer layer, like hydrogen or iron, absorbing specific frequencies of light. By carefully measuring the width of each dark band, astronomers can determine just how much hydrogen, iron, calcium, and other elements are present in a distant star. ...

. Open Systems Centre   . olein@cplire.ru . 2 . To Open System Principles . Scientific researches. Spectrum of demands   . Heterogeneous computing environment (GRID) . Open Systems Principles . Spectrum of computing . “Transparency” of environment

C C C C C C lass lass lass lass lass lass 1 2 3 4 5 6 Introduction, Background Solar System Stars Galaxies Cosmology Special Topics Class 1 Introduction, Background History of Modern Astronomy The Night Sky, Eclipses and the Seasons Kepler's Laws Newtonian Gravity General Relativity Matter and Light T lescopes e 1. ... Kirchoff's Laws trum Emission Line Spectrum 2. A low-density, hot gas emits light whose spectrum consists of a series of bright emission lines. ... Absorption Spectrum 3. ...

... L.V.Zotov , C. M. Bizouard Envelope calculation () () () E() L.V.Zotov , C. M. Bizouard Envelope calculation () () () E() L.V.Zotov , C. M. Bizouard Amplitude model and forecast 3-layer Neural Network with (7, 7, 1) neurons L.V.Zotov , C. M. Bizouard Phase model and forecast 3-layer Neural Network with (7, 7, 1) neurons L.V.Zotov , C. M. Bizouard Phase and amplitude models ~ Chandler ...

Supernova 2000eo in MCG -2-9-3 . This page is devoted to information on Supernova 2000eo in MCG -2-9-3 Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the Supernova links web page. This supernova was originally discovered on a deep scan by Nearby Galaxy Supernova Search (NGSS) at magnitude 19.2. ... NGSS image . ... LOSS image . ... 15.5: . ...

... Предлагается способ радиометрических измерений энергетических параметров широкополосного сигнала в континууме, основанный на преобразовании шумового сигнала в широкополосном приемном канале в последовательности цифровых выборок и вычислении методом быстрого преобразования Фурье энергетического спектра, по которому определяются мощность и шумовая температура исследуемого сигнала. ... The Spectrum Method of Radio Meter Measurements with Radio Interferences Selection . ...

Обзоры hep-ph: тематический рубрикатор . Связанные состония в теории поля и спектр адронов . ... Классические решения в SU(2) и SU(3) теориях Янга-Миллса и массовый спектр тяжелых адронов . ... Похожесть доходит до того, что авторы задаются вопросом: а может быть, классическую неабелевую теорию поля можно свести к простому описанию набора невзаимодекйствующих фотоно-подобных частиц? Авторы отмечают, что для случая глюонного поля одно из решений имеет вид кулоновского потенциала. ...

... The project assumes creation of an international space observatory - the interferometer "Earth - Space - Space" in order to perform of astronomical investigations in millimeter, submillimeter and infrared regions with extremely high sensitivity (to a few nanoJanskies units of flux density in continuum spectrum) and extremely high angular resolution (to a parts of microsecond of arc or, possibly, nanosecond). ... radio-interferometric channels of the system "Space - Space", region 0.2 - 3 mm; . ...

... Authors: Adam G. Riess et al. !!! astro-ph/0402418 Сильная широкая линия поглощения в рентгеновском спектре близкой одиночной нейтронной звезды RX J1605.3+3249 (A Strong, Broad Absorption Feature in the X-ray Spectrum of the Nearby Neutron Star RX J1605.3+3249) . ... Authors: S. Komossa et al. astro-ph/0402095 Построение трехмерной карты распределения темного вещества по данным о слабом линзировании в обзоре COMBO-17 (Mapping the 3-D dark matter with weak lensing in COMBO-17) . ...

... Module Spectrum was launched from Baikonur on May 20, 1995 by the LV Proton-K. The mass of the module at the launch was 19640 kg. ... The area of the main panels of the SB is 2*27 m2 (6.9 kW); the area of the additional panels of the SB is 2*38 m2 (9.3 kW). NiCd batteries of capacitance 360 Ah are set up on the module. ... Later the task was corrected and module was reaimed at the supporting the service systems of the complex in the working condition. ...

Planar polymers of С 60 undergo irreversible transformations at high pressure , related with formation of new polymer bonds perpendicular to the two-dimensional polymer planes . It is established that tetragonal (2D-T) polymer transforms into a new three-dimensional polymer phase at pressure ~20 GPa ( Fig . ... The new phase is characterized by chaotic formation of polymer bonds between molecules , belonging to neighboring planar polymer planes . ...

... Solanki S. K. Small-scale solar magnetic fields: An overview // Space Sky . ... Fe I 5247,1 5250,2 е, Fe I 6301,5 6302,5 е. ), . ... Lvm 5250 , 6301 ­ . ... k, rv- (rvw), rv- - (rvf). , rvo = rvf + k* rvw, rvo ­ . ... 2 , Lvm, [6] е 5247 40,5 5250 58,5 6301 67 6302 73 Lvm, [5] 40,8 40,8 64,8 58 Lvm, k=0,8 40,8 53,2 65,5 65 Lvm, k=-0,8 39 61,2 69,5 80 Lvm, k=3,0 40,8 44,8 65 61 Lvm, k=-3,0 27,2 53,5 65,2 49,5 80 86 If*f, rvo = (rvf + k*rvw)/ [1 + (1-f)/f *Ip/If], k = (Ip*p)/(If*f) = 0,72p/f (3) (2) ....

. Russian Version [ MS-Win ] . [ News ] . [ Satellite data ] . [ SMIS ] . [ ] . The program is intended for spectral and correlation analysis of satellite images. It contains an large set of spectral and spatial filters. It may be applied for interpolation and data analysis in areas with incomplete information. It allows for approximation of spectrum and correlation functions. Price . Back to SMIS Home Page .

... Bad Astronomy . Misconceptions . ... Keep Bad Astronomy close to your heart, and help make me filthy rich. ... Comets are not "dirty snowballs" . ... Miscellaneous nonsense . ... McCanney's Claim #1: Comets are not dirty iceballs, but hot, rocky bodies with no water. The core claim McCanney makes is that comets are not frozen balls of dirt and ice, as mainstream science would have you think. ... Conclusion: Comets are cold balls of ice, not hot and dry. ... 2008 Phil Plait. ...

... Информация Руководство и преподаватели Агафонов Андрей Николаевич . ... Публикации . ... Control of transverse mode spectrum of Novosibirsk free electron laser radiation // Applied Optics. ... Агафонов А.Н. , Володкин Борис Олегович , Кавеев А. К. и др. Фокусировка излучения новосибирского лазера терагерцового диапазона (novofel) в соосный отрезок // Компьютерная оптика. 2015. том 39, ?1. ... Агафонов А.Н. , Володкин Б.О. , Кавеев Андрей Камильевич и др. ... 2013. ... 2012. ...

... 2003). ... RHESSI, (HXR) , HXR- . ... 15) n = n0 1+(bm - b)l2 (15) (1) (14), bl(bm - b) , ME = ME0 1+(bm - b)l2 33 1 2007 (16) 67 ME0 - , : ME0 = np0 Ne0 . ... ME = ME0 1+(bm - b) (18) (17) ME/ME0 6 5 4 a 3 b 2 c 1 1.0 0.8 0.6 I (З) a 60 40 20 0 0.2 b c 0.4 0.6 (b- 1)/(bm - 1) 0.8 1.0 0.4 0.2 0 () 100 80 (17), (18) . ... 33 1 2007 5* 68 , 1.0 () 0.8 шгкгЭ HXR-ЫСЮл~ТЬЫfl, з 10-8 йгкгЬА в-1 ЭЧ-1 0.6 0.4 0.2 0 1.0 8 (З) 6 a b c 0.8 0.6 l 0.4 0.2 0 a 4 2 b c 0 0.2 0.4 0.6 (b - 1)/(bm - 1) 0.8 1.0 . ...

Communications For Your Astronomy Event . Articles | ... The FCC agreed and in 1996 created the Family Radio Service (FRS) as one of the Citizens Band Radio Services. ... You are provided authority to operate a FRS unit in places where the FCC regulates radio communications as long as you use only an unmodified FCC certified FRS unit. ... Frequencies Used 462.5625-467.7125 MHz . FRS Channel Plan . ... 0.5 Watts . ... www.astronomy.net . ... dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...