On line simulation in ALMA Software Robert Lucas ALMA Simulation workshop Summary · · · · · · Need for hardware simulation for software testing Requirements for on-line simulation A Shared Simulator Limitations Current capabilities Further work ALMA Simulation workshop 2 Need for on-line simulation · Main motivation is to test software ­ At the subsystem level: simulate the ... ALMA Simulation workshop 8 Actual scope? ... ALMA Simulation workshop 11 Further work? ...

The Agile ICC computer (nimble) contains a high-accuracy GPS-synchronized timer card that emits pulses that trigger readout of the Agile camera when run in external synch mode. ... The recommended configuration for Agile has no GPS receiver (see 1 PPS Vs. The Built-In GPS Receiver below). ... Using external 1 PPS with on a GPS receiver mode is not fully supported, in that the timer card's firmware has been programmed to assume a GPS, but the tech support person claimed it would work. ...

Astronotes Armagh Planetarium's Stellar Blog! ... Armagh Planetarium . ... Space Flight . ... By admin December 16, 2015 Posted in: Armagh Planetarium . There have been so many fantastic entries this year that the judges have struggled to pick the winners, so in the spirit of Christmas we now have four overall winners that have won a trip for their class to come to the planetarium and 28 runners up who have each won an individual family pass to visit the planetarium! ... Subscribe to Astronotes . ...

... The thesis was titled "Numerical modeling of chemical evolution of galaxies". ... Kurbatov E.P., Kinematic effects of velocity fluctuations for the dark-halo population in a LmabdaCDM model , 2014 Astronomy Reports, Vol. ... ADS Preprint . ... Kurbatov E.P., The influence of OB associations decay upon evolution of dwarf galaxies , 2010 Astronomy Reports, Vol. ... Kurbatov E.P., Tutukov A.V., Shustov B.M., Evolution of galaxies and the Tully-Fisher relation , 2005 Astronomy Reports, Vol. ...

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Stellarium 0.12.3 . ... Classes . ... TuiNodeFloat Class Reference . Allows navigation but also editing of a float value. ... TuiNodeFloat (const QString &text, QObject *receiver, const char *method, float defValue, float min, float max, float inc, TuiNode *parent=NULL, TuiNode *prev=NULL) . Create a TuiNodeFloat node. ... virtual TuiNodeResponse љ . ... TuiNode (const QString &text, TuiNode *parent=NULL, TuiNode *prev=NULL) . ... virtual TuiNode *љ . ... the default value for the node . ...

... We received the SASS output for the HRI observation of 3C 120 (a highly variable radio galaxy with a prominent jet leaving the core at PA ) and smoothed the data with a Gaussian of FWHM = 3 '' ( Figure 13.1 ). ... The results are shown in Figure 13.2 . ... The FWHM of the original data ( Figure 13.1 ) is 11.8 (PA ); after dewobbling ( Figure 13.2 ) the width of the 50% contour is 7.6 . ... Figure 13.1 : The original data, smoothed with a Gaussian of FWHM = 3 . ...

. S. G. Pugacheva and V. V. Shevchenko, Sternberg State Astronomical Institute, Moscow University, 13 Universitetsky pr., 119992 Moscow, Russia, pugach@sai.msu.ru . Pugacheva LPS 41.pdf - 208K б . Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow, 119992 Russia . Received December 21, 2009 . SSR-10(Busarev).pdf - 239 KB . V. V. Busarev . Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow, 119992 Russia . Received December 21, 2009 . SSR-11(Busarev).pdf - 204 KB .

Towards celestial sources above 1 THz with a heterodyne receiver based on a hot-electron bolometer mixer Sergey Ryabchun, Ivan Tretyakov, Matvey Finkel, Natalia Kaurova, Boris Voronov and Gregory Gol'tsman HOT-ELECTRON BOLOMETER (HEB) MIXER Scient ific and Educatio nal Radiophysics Center Mo scow State Pedago gical University Mo scow, Russia FIRST GROUND-BASED OBSERVATION WITH HEB MIXERS BEYOND 1 THz Submillimeter Telescope ...

... The first comparison of the SOHO/EIT and mosaic TRACE modified images at the same wavelength (171 A) received after the SOHO repair. There is a minute coincidence of the large-scale EUV chains on these images received with two different space observatories SOHO (a) and TRACE (b). ... Back to the page of the SOHO/EIT and TRACE chains . Back to the parent page . ...

INFRARED FOURIER-SPECTROMETER SICH-F . ... Instrument work regimes: 1) Inside. 2) Calibration at inside standard sources 2 - 4 times per a rotation. 3) Calibration at "free space" 2 - 4 times per a rotation. 4) Infrared radiation measuring 10 - 40 min. per a rotation. ... Spectrometer consists of the photodetector block and the block of signal processing and control. ... Diagnostic information and attach data will transfer by state telemetric channels. ... Detector temperature. ...

... B.V. Somov . head of the department . ... room 80 . ... senior research felow . ... research felow . ... research fellow . ... Our department performes the following most perspective studies: . Special analytical and numerical experimental investigations of the solar plasma involved in the magnetic reconnection process at the Sun. ... Head of the seminar: Prof. B.V. Somov. ... 27 September 2013 The Solar Physics Department was visited by journalists of the leading Russian TV channel "Vesti-1". ...

... 8, ``Celestial Mechanics'', 2002 First results of GPS orbit determination with GRAPE package using a square--root information filter M. O. Keshin Institute of Applied Astronomy, St. Petersburg, Russia The zero--differenced carrier phase measurements contain the distance be­ tween the phase centres of receiver and transmitter antennas biased by unknown integer number of cycles (phase ambiguities). ... In the case of GPS the problem of solar radiation pressure modelling is of primary importance. ...

... Up: Data Pipelines . ... The Data Handling System (DHS), developed for the Gemini project by the Canadian Astronomy Data Centre, accepts observational data from multiple sources. There may be data descriptions, image data in chunks (to be composed into a single image), and multiple images for one dataset, all being received at different times. ... DHS is data-driven and is composed of a collection of servers that work together to act on any data it receives from any Gemini principal system. ...

... Bad Astronomy . ... Mad Science . ... Keep Bad Astronomy close to your heart, and help make me filthy rich. ... Bubbles as in the bubbles found in soda, soft drinks, all flow upwards,when shaken .Is it possible that it would ever flow downwards? ... They "know" which way down is because that is the way gravity pulls them, and they tend to flow away from that direction. ... It is the acceleration of gravity that the bubbles feel, and they flow in the other direction. ... 2008 Phil Plait. ...

... You may write to me if you have questions. ... Let G be a locally compact abelian group, H be a compact open subgroup, and let f L1 (G). Fix a Haar measure µ on G to define the Fourier transform f : G C. a) If f (g ) = 0 for all g H , show f : G C is constant on H -cosets in G: f ( ) = f () if H . ... Let p be a prime. p 1 |y |2 1+1/p p a) In the topological group R в Qp , show Z (embedded diagonally) is discrete but not co-compact and Z[1/p] (embedded diagonally) is both discrete and cocompact. ...

... Under conditions of the Earth gravitation we are using the method of semi-natural simulation of linear accelerations in the centrifuges with a mobile cab for simulation of G-loads, originating in a space flight. ... The major factor of the orbital flight, affecting a cosmonaut, is a weightlessness state, which causes essential changes in cardiovascular and vestibular systems operation. ... Under the Earth conditions you can "execute" a short-term space flight according to the following cyclogram: . ...

... COMPUTER SIMULATION OF RADI