... Bad Astronomy . ... I think I will break from my usual format of Bad Astronomy/ Good Astronomy by saying that the way we define seasons currently is not strictly bad, but I feel (in my opinion!) that it could be better. The definition of when the seasons begin is at the moment of solstice or equinox; that is, winter (in the north) starts on December 22 nd and summer starts on June 22 nd . ... Now imagine breaking up the Sun's 46 degree up-and-down yearly swing into 1 day intervals. ...

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First results of X/S and X/Ka-band catalog combinations with full covariance information Andreas Iddink , Christopher Jacobs, Thomas Artz, Axel Nothnagel 22.09.2014 First results of S/X and X/Ka-band catalog combinations with full covariance information Andreas Iddink ­ 22.09.2014 Motivation Features of the ICRF2 ICRF2 (Defining- Sources ) 3414 ... Step: Import of the X/Ka catalog with full covariance information (Data provided by Christopher Jacobs et al. ...

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... 18c. Work . ... The concept of Work is closely related to that of energy. ... Suppose we lift a weight A of mass m a distance h (for height) from the floor to the table (Figure 1). ... That, however, is just the potential energy added to the weight! ... Energy is always preserved but--as seen in an earlier section--not always in a usable form. ... Because the trains are linked, when one goes up, the other descends, and by giving up its potential energy, it helps pull the other one upwards. ...

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... IX Title "Bulkmail::DummyServer 3pm" .TH Bulkmail::DummyServer 3pm "2003-12-22" "perl v5.8.4" "User Contributed Perl Documentation" .SH "NAME" Mail::Bulkmail::DummyServer \- dummy class for dummy server objects .SH "AUTHOR" .IX Header "AUTHOR" Jim Thomason, jim@jimandkoka.com .SH "DESCRIPTION" .IX Header "DESCRIPTION" Mail::Bulkmail::DummyServer is a drop in replacement for Mail::Bulkmail::Server. ... Mail::Bulkmail::DummyServer is distributed under the terms of the Perl Artistic License. ...

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Astronotes Armagh Planetarium's Stellar Blog! ... Space Flight . ... December . ... By admin December 9, 2012 Posted in: Armagh Planetarium . Patrick Alfred Caldwell-Moore was born in 1923 and began his life-long interest in astronomy from a very early age. ... Demonstrating a good-natured wit, Moore impressed both viewers and programme makers. ... In 1965 Patrick Moore was invited to Northern Ireland to be the first director of Armagh Planetarium which was already under construction. ...

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and 42 % 27-11-1999 Andr\'as Holl % 2.31: 02-05-2001 % % Konkoly Observatory, Budapest, Hungary % Use the following documentstyle definition : % \documentstyle[twoside, ibvs2, epsf]{article} % or % \documentstyle[twoside]{article} % \input ibvs2.sty % \input epsf.sty % epsf is only needed for figures % IBVS.STY screen message \ typeout {} \ typeout {IBVS.STY Ver. 2.31 - 02-05-2001 } \ typeout {Information Bulletin on Variable Stars - Konkoly Observatory} \ ...

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... Proposed location of the new generation Russian VLBI network radio telescopes Kaliningrad St. Petersburg Zelenchukskaya (Zc) Badary (Bd) Ussurijsk Working frequency bands for the new generation Russian VLBI network S X Ka 2.2 2.6 7.0 9.5 27 33 F, GHz Data acquisition parameters 4 frequency bands : 512 MHz bandwidth x 2 polarisations or 1024 MHz bandwidth x 1 polarisation 2-bit sampling ...

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Supernova 2007uy and 2008D in NGC 2770 . This page is devoted to information on Supernova 2007uy and Supernova 2008D in NGC 2770 . ... Information on the original web pages for many of these images can be found on the updates and links web pages. 2007uy was discovered by Yoji Hirose (Japan)). ... 2008D was discovered by the Swift/XRT satellite which was then observing 2007uy , and announced by Lick Observatory Supernova Search (USA). ... SNWeb has a 2007uy page and 2008D page . ... JM Llapasset . ...

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Atm 2 ospheric time constant with MASS and FADE 0 A. Tokovinin CTIO, Chile Adaptive Optics time constant 0 = 0.314 r0/V0 = 0.057 6/5 [ Cn2(h) V5/3(h) dh MASS time constant: 0, MASS, Numerical simulation 1. Set turbulent layer strength (seeing) & sp. response Definition (1 rad phase difference between wavefronts at t= 0) ] 3/5 = 0.175 (2 DESI ) 3/5 ; 2 DESI = < [ IA(1ms)/ IA(3ms) ] >2 0, MASS, This is an approximation! ... The MASS method is approximate! ...

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RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . Principle of generation of radio images General information Main characteristics of the Radio telescope Observing programs General view of the antenna array Main research areas Radio telescope's beam Receiving systems Main characteristics of the base receiving-recording complex Calibrations Data archive and databases ... Solar radio images are generated by beams oriented within the SSRT field of view (90'). ...

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. Language [RU/EN] Search: . Home . UP . Research . Projects . Services . Info . News . Events . Personal . Archive . Ionosphere and radiowave propagation: structure . The main page . Information . Publications: . 2011 - 2015 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2000 - 2004 . 1995 - 1999 . Participation in International symposiums and conferences: . 2013 - 2015 . 2011 - 2012 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2002 - 2004 . N.V. Pushkov . 09/04/2016 23:52 MSK . webmaster@izmiran.ru .

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... Управление полета . Полет "Союз ТМА-13" . Экипаж "Союз ТМА-13" . Эксперименты . ... Оценка атрофии глубоко расположенных мышц человека в условиях невесомости по регистрации субъективных болевых ощущений в области поясницы, испытываемых астронавтом в течение дня. ... Исследование влияния микрогравитации на роговицу глаза. ... Ежедн. с 14.10 . ... УКП -5 мин . ... 14.10 - перенос контейнера из ТК 'Союз ТМА-13', размещение на месте экспонирования и *фото . ... УКП - 1 час 20 мин . ...

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... Basics of Group Theory Definition 1. A group G is a (finite or infinite) set of elements g1 , g2 , g3 , . ... Definition 2. ... Each element of a finite group may be represented as a power or product of powers of a certain finite number of elements cal led generators of the group. ... Point Groups Any transformation which brings a body into coincidence with itself can be decomposed into elementary transformations: 1) rotation about an axis, 2) reflection in a plane, 3) translation by some vector. ...

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wavelet-transformation of the signal % program is written 27.01.2009 by L.V. Zotov clear; N_signal =1024; % generating two-sin signal for (k=1:1: N_signal ) if k ( N_signal /2) garm (k)=5*sin(2*pi/20*(k-1)); else garm (k)=5*sin(2*pi/50*(k-1)); end ; end ; plot ( garm ); % ARMA process generating ar(1)= 0.5 * randn (1); ar(2)=-0.2*ar(1)+ 0.5 * randn (1); for (i=3:1: N_signal ) ar(i)=0.9*ar(i-1)-0.7*ar(i-2)+ ...

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CALCSYM - complex evaluator . ... CALCSYM.exe and CALCSYMi.exe will allow you to obtain numeric solution for *.out file generated by both CIRSYM and MATSYM programs (computation of freqency responces, unknowns, determinants, sensitivity analysis etc.. ... Setup file name for CALCSYM is "setup.cal". ... CALCSYMi.exe will allow you to work with long double over the range from 3.4*E-4932 to 3.4*E+4932. ... To calculate, run CALCSYM.exe and enter "file_name.OUT" or click on the "ENTER" (in "OUT" case). ...

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... NASA] Космическое агентство NASA сформулировало новую программу по созданию космического корабля многоразового использования второго поколения (Second Generation Reusable Launch Vehicle, 2nd Generation RLV), который должен быть гораздо безопаснее и дешевле современных ракет. Предполагается, что полеты этих кораблей начнутся в 2010 г. Напомним, что нынешние "шаттлы" считаются кораблями первого поколения. ... другие статьи .. ...

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... STScI has undertaken a project to place all HST keyword information in one source, the keyword database, and to provide a mecha­ nism for making this keyword information accessible to all HST users, the keyword dictionary, which is a WWW interface to the keyword database. ... Along with form­ ing the headers for the science data, most keyword values are ingested into HST archive catalog fields where they are accessible for archive searches and data characterization. ...

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• About this document ...

Russian . ... Very Early Universe: inflation, generation of primordial perturbations, preheating . Very Early Universe: inflation, generation of initial perturbations, preheating . Cosmic Microwave Background Radiation: anisotropy and polarization . ... Dark Energy and Dark Matter models . High Energy Astrophysics: accretion discs, cosmic rays, gamma-ray bursts . ... Astrophysics of black holes and wormholes . ...

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... Parameter Spec Measurement Technique: Wavelength = 355nm (Visual confirmation) Energy = 30 uJ, 160-180 mJ (4025 pulses), 40 uJ (micropulse) Pulse Duration = 10 ms (Measured at 10 ms on an oscilloscope) Micropulse Width = 70ps IR, = 50 ps UV (Autocorrelator to measure IR pulse waveform Temporal Profile - flat envelope) Measured at 10 ms on an oscilloscope. ... Burn Paper measurement) Repetition Rate = 10 Hz/402.5 MHz Oscilloscope Shot to Shot Stability = 3% RMS for pulse envelope. ...

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