эффектов галактических и солнечных космических лучей методом наземного мониторинга ' в рам ках программы фундаментальных исследований Президиума Российской академии наук ?6 Нейтринная физика за 2006 г. В результате выполнения данного проекта осуществлялась непрерывная регистрация интенсивности КЛ на Саянском спектрографическом ... Известия РАН, серия физическая (в печати). ... Координатор http :// www . ...

Atlas of the Arcturus MgH line's families spectrum* O. M. Ivanyuk, Ya. V. Pavlenko Atlas consists on three parts: The first part ­ is a spectrum atlas in range from 4925е till 5225е that covers MgH A -X 0-0 , MgH A-X 1-1 and MgH A-X 2-2 line's families The second part of atlas shows range from 5375е till 5625е in accordance with MgH A-X 0-1 and MgH A-X 1-2 families And the third ...

Kholtygin A.F., Galazutdinov G.A., Burlakova T.E., Valyavin G.G., Fabrika S.N., Lee B.-C. Microvariability of Line Profiles in the Spectrum of the Star iota Her . Astronomy Reports, 50 , 230-231 ( 2006 ) Original Russian Text published in Astronomicheskii Zhurnal, 83 , No. 3, pp. ... We present the results of a search for and analysis of line-profile variations in the spectrum of the star iota Her. ... Evidence was found for cyclic variations of the lines, with periods from 7 hour to 2.9 day. ...

... DIAGNOSTICS OF IONOSPHERIC IRREGULARITY SPECTRUM USING MEASUREMENTS OF RADIO WAVE ANOMALOUS ATTENUATION UNDER VERTICAL SOUNDING . ... The selected experimental data are characterized by a high average level of attenuation of a signal of vertical sounding (10 dB and above), which cannot be caused by collisional absorption of radio waves (practically absent in a dark time of day) and, hence, being a consequence of scattering on random irregularities. ... ATTENUATION OF A VERTICAL SOUNDING SIGNAL . ...

Superconducting Integrated Submm Spectrometer for Laboratory Applications Specification: · Input frequency range : 200 ­ 700 GHz (covered by four exchangeable sensor modules each one covering range of about 100-150 GHz ); · Output frequency (IF) range : 1-2 GHz · Receiver noise temperature: below 500 K (direct ... The SIR chip is a superconducting integrated circuit comprising a quantum-noise-limited SIS mixer and a tunable Josephson local oscillator (LO). ...

... OF ROCKET SPACE TECHNOLOGY DEVELOPMENT . OKB1 - TSKBEM - NPO ENERGIA - S.P.KOROLEV RSC ENERGIA . December 7, 1998 . ... Demonstration start of the Zenith-3SL launch vehicle under the Sea Launch program. ... Launch into a target orbit of the Yamal-100 communication satellite possessing improved technical characteristics. S.P.Korolev RSC Energia restarted its activity in development of communication satellites on new technical basis and other automatic space vehicles on their basis. ...

... 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 . ...

... 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 ...

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. ...

. Home . - . Overview . Glossary . Observing . Exposure Time Calculator (ETC) . Survey processing . Pictures . Publications . - . External Links . ESO - Public Surveys . near IR surveys . DENIS . 2MASS . UKIDSS (in north) . Site and Enclosure . Telescope . Mirrors . Optics . Camera . Focal Plane array . VISTA images from press releases . @PPARC . @ESO . Menu of 23/10/2012 . Page updated insert date edited by J.P.Emerson to whom comments should be sent . [ ESO ][ VISTA Home ]

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: . ...

You may see figures of this paper below... or download the whole paper in PostScript or LaTeX source , everything compressed by ZIP. LaTeX notes: you would need some specific LaTeX styles . See CS-11 HomePage for more. Figures are in EPS (Encapsulated PostScript) format to be inserted using software like dvips . You can download these files via ftp. If you use GIF format, choose "Save Image As..." on the images below, or click here: first and second . Figure 1. ...

1975 LUMAM v.18 7/11/2002 5:49 PM Page 1 LUMAM System Diagram DIGITAL CAMERA C-MOUNT CCD CAMERA 35MM CAMERA EKW-6.3LU EKW-10LU EKW-15LU EM-15LU CT4 EYEPIECES VA-T1LU EXCITATION FILTER EMISSION FILTER VA-V20LU VA-F20LU HB-45LU HT-45LU FILTER CUBE INSERTS WITH DICHROIC BEAM SPLITTER FILTER SLIDERS FOR REFLECTED LIGHT MERCURY ILLUMINATOR FOR HOUSING & ASSEMBLY LUMAM INFINITY-CORRECTED PLAN FLUORITE AND PLAN ACHROMAT OBJECTIVE SERIES C-BFLU MERCURY POWER SUPPLY C-PHDLU CONTRAST FILTERS FOR TRANSMITTED LIGHT

Program e10_up_y; {y=10**y} Uses crt; var Cod,k,m,n : word; InpF , OutF : text; X,Y, Y10 : real; str12 : string; begin clrscr; TextColor(15); for k := 1 to ParamCount do WriteLn ( ParamStr (k)); if ParamStr (1) '' then for m:=1 to ParamCount do begin Assign ( InpF , ParamStr (m)); Reset( InpF ); { Assign ( InpF ,'D:\(DB_GLE)\DataWork+'+ ParamStr (m)); Reset( InpF );} str12 := ParamStr (m); Delete( ...

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; . ...

... 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. ...

... 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) ....