... TICTOC is a cookbook program that demonstrates how to use Toolkit routines to convert between different time representations. ... UTC . is a string representation of Universal Time Coordinated, which may be in calendar, day of year, or Julian date format. ... Enter Y or N): Y Example UTC time : 86-365//12:00 Corresponding ET : -410313544.816091 UTC calendar format : 1986 DEC 31 12:00:00.000 UTC day of year format: 1986-365 // 12:00:00.000 UTC Julian date format: JD 2446796.000 Continue? ...

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• Conclusions
• Mathematical Analysis of the Iterative/Recursive Algorithm
• The Hubble Deep Field - drizzling

Next: The Scenario Machine: Operational Up: Evolution of Magnetic Rotators Previous: Ejector-propeller hysteresis . ... The length of this segment is determined by the eccentricity. ... In this case no hysteresis occurs and transitions E -- P and the reverse take place in symmetrical points of the orbit. ... Here EP means a mixed state of the rotator at which it is in the ejector state during one part of the orbit, and in the propeller state during the rest of the orbital cycle. ...

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• Presentation of the results

REPORT ON PIERRE DELIGNE FELLOWSHIP, 2010 SERGEY OBLEZIN During 2010 I have been working on developing a representation theory approach to mirror symmetry and quantum cohomology of homogeneous spaces, associated to Lie groups of classical type. According to Givental the glN -Whittaker functions, being solutions to the quantum cohomology D-module QH (FlN ) of the complete flag variety FlN = GLN (C)/B , describe the corresponding equivariant Gromov-Witten invariants of FlN . ... J. (2010). ...

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• http://www.mccme.ru/dfc/2010/reports/2013-Kuyumzhiyan_Report.pdf
• http://www.mccme.ru/dfc/2009/reports/2011-Oblezin.pdf

... Especially necessary for an assessment of the calibration reliability of simulations of the different observing modes (still to be performed by the XMM-Newton calibration teams) was the closure of the loop between simulation and data analysis. This has been done complementing the SciSim release with the release of 90 specific SciSim calibration files included in the SciSim CCF tarfile , together with the corresponding Calibration Index file CCF_scisim.cif. ... Pages maintained by SAS librarian . ...

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• Analysis options
• Processing OM Image mode data
• Different types of detector map

... Slide 2 . ... Smooth Accretion of Intergalactic Gas . Mergers and Satellite Accretion . Galactic Fountain Material . HIPASS = HI Parkes All-Sky Survey . A typical HIPASS data cube . HIPASS was designed to be an extragalactic survey . ... Different types of HVCs in different environments? ... HVCs and Galactic Emission . ...

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• Arecibo Observatory at the Childrenт??s Museum in San Juan National Astronomy
• Making Maps: Example + Animation

... The gravitational lens effect of the red, foreground, elliptical galaxy visible near image center creates a cloverleaf image of the single distant quasar. ... NGC 1850: Gas Clouds and Star Clusters . ... Globular clusters only 40 millions of years old can still be found in the neighboring LMC galaxy, though, but perhaps none so unusual as NGC 1850. The Coma Cluster of Galaxies . ... Stars Without Galaxies . ... Galaxies are made up of stars, but are all stars found within galaxies? ... March . ...

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Next: Echelle Reduction Method Up: No Title Previous: Example . This Chapter provides the basic information necessary to understand the echelle љ package implemented in MIDAS . ... Tutorial examples are available in the system (command TUTORIAL/ECHELLE ) and are also included in the Appendix so that users without previous experience in MIDAS could become familiar with the calibration procedures. ... Reduction steps which are not specific to echelle spectra are described in more detail in Chapter . ...

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• HyperLEDA: documentation
• Performing Batch Reduction
• CCD Image Quality - PixelVision

Time Standard and Ensemble Pulsar Time Scale Ding Chen, George & Dick, Bill 20100928, Orange National Time Service Center. ... Ensemble Pulsar Time Scale(EPT) : (TAI - EPT ) = k = ( 2 k k =1 N ^ k (TAI - PTk ) + 2 z ,k ( T )) -2 PPTA is the best project to establish the new independent ensemble time scale which will take contribution to both GW detection and BIPM. ... Ensemble Pulsar Time Scale is more stable than the AT of some clock laboratory on long term scale. ...

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• Australia Telescope National Facility
• Weighting
• casacore: casa/BasicMath/Functors.h File Reference

... Next: An IRAF-Independent Interface Up: Software Systems Previous: A New PROS . ... We present a high-level representation of the packages and tasks within IRAF/PROS. ... We have produced a high-level overview of PROS. ... The incremental stages were the short-term goals: a project overview diagram (i.e., an organizational diagram of software modules); high-level diagram (i.e., a bubble diagram of each module in the system); and unifying element tables (i.e., tables of task vs. software attributes)....

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• Synthetic Images of the Solar Corona from Octree Representation of 3-D Electron
• ADASS 2003 Conference Proceedings
• Recognition of Anomalous Events

... 2007 June 2 . 3D Full Moon . ... Explanation: Get out your red/blue glasses and check out this satisfying stereo anaglyph of the Full Moon. ... Regardless of your preferred technique for stereo viewing , the 3D effect comes from combining pictures of the same scene taken at different angles -- mimicking the slightly different perspective of each eye. Perhaps surprisingly for Earthdwellers , getting two pictures of the Full Moon from different angles only requires a little patience. ...

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• APOD: 2007 March 6 - Saturn from Above
• APOD: 2013 October 21 - Saturn from Above
• APOD: 2009 November 12 - Art and Science in NGC 918

The following figures show the behaviour of the efficiency factors Q ext , Q sca , Q abs as well as albedo and asymmetry parameter g for porous particles. ... These optical characteristics are compared with results of Lorenz-Mie calculations for corresponding n -layered spheres. ... factors . Qext(x) . Qsca(x) . ... Qabs (x) . ... albedo (x) . ... Henning, Modelling the optical properties of composite and porous interstellar grains, Astronomy and Astrophysics , 429 , 371-381, 2005. ...

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• Database of Optical Properties -- Level: subsubpage
• Rayleigh-Debye-Gans approximation (RDG)
• Database of Optical Constants -- Level: welcome

... The value of tile-size, NW , may be thought of as a sixth coordinate axis in the chirplet transform parameter space - TF-area. Including this sixth coordinate axis provides us with a hierarchical (multi-resolution) CCT. ... Various 2- D slices through the multiresolution CCT may correspond to useful tilings of the TF plane with true parallelograms (true to the extent that the DPSS define a truly rectangular region in the TF plane). ...

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• Specifications
• Y. Meyer, 1993, Wavelets: Algorithms and Applications, S.I.A.M.
• Different Fortran standards

. The polar diagram shows the spacecraft corrected geomagnetic co-ordinates : co-latitude - local time . The geomagnetic co-latitude in the range (10 ° , 50 ° ) is shown with 10 ° step. The geomagnetic local time meridians correspond to 6, 12 and 18 hours. The different colours are used for each of the 4 spacecraft. On the plot the SC names are shown by the corresponding colours.

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• INTERBALL Tail Probe flight longterm situation analysis 1995 - 2000
• Situation investigation for using during IACG/ISTP Campaign 2 scheduling
• How can you investigate the SCA-1 measurements.

In this chapter we will consider an example of visual expert system written on the Actor Prolog language. ... There are a lot of methods of oil field bed stimulation that increase output of the oil production: thermal, physical-chemical, gas, microbiological, and others. ... Fig. ... The Top-Most diagram consists of three blocks: the "Describe parameters of hydrocarbon field" block, the "Check adaptability of existed methods of oil production" block, and the "Display solution" block. ... Gas methods. ...

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• Atmospheric influence on the different radioengineering systems functioning.
• Getting Started in Actor Prolog. 3D Web Site.
• Actor Prolog User Guide. SADT.

To construct two-dimension distribution of minor planets user should specify elements/ parameters/ function that will be plotted as abscissas and ordinates. In three-dimension case one should add to them the element plotted on Z axis. ... Though you may choose elements plotted along different axes at will, often there is good reason to plot such elements as a, n, or n" along X axis (two-dimension distributions) and to plot them along Y axis in three-dimension case. ...

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• Keywords_146
• AY (preface)
• Keywords_347

Stellar Clusters are very useful laboratories for empirically studying stellar evolution. ... All cluster stars are at the same distance . All cluster stars have the same physical age . ... CM diagram Young Cluster In this case we see the Main Sequence fully represented. The blue dots represent massive stars with short main sequence lifetimes. ... Thus, identifying the most massive star which is still on the main sequence is an effective means of determining the age of a stellar cluster. ...

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• Astronomy HyperText Book
• First Steps to the Renaissance
• Venus and Mars

National Academy of Sciences of Ukraine Institute of Physics of NAS of Ukraine European Profiles A.E. (Greece) Institute of Physics of the University of Tartu (Estonia) University of Turin (Italy) Pierre and Marie Curie University (France) Ivan Franko National University of Lviv (Ukraine) 1918 International research and practice conference: NANOTECHNOLOGY AND NANOMATERIALS NANO-2015 26 ­29 August 2015 Lviv, Ukraine Great Conference Hall of Ivan Franko National University of Lviv Dear colleagues! ...

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... Unlike the previous digital-only Messages, Arecibo-1974 and Evpatoria-1999, the TAM has complex, three-section structure with different forms of information. Section 1 represents coherent sounding radio signal with slow Doppler wavelength tuning to imitate transmission from Sun's center. ... Section 2 is an analog information and represents musical melodies, performed on the Theremin. ... There were seven musical compositions in the 1st Theremin Concert for Aliens. ...

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• http://lnfm1.sai.msu.ru/SETI/eng/articles/sokfro.html
• Data bases of Natural Satellites. Documentation. Structure
• Photos from the latest lunar eclipse (march 2007)

SAI VO . ... SAI CAS . ... Access . ... We present the results of the development of Sternberg Astronomical Institute Catalog Access Services (SAI CAS) project - the first and the only project in Russia, which provides online access to the major astronomical catalogues and different services on top of them. ... SAI CAS is an open-source implementation of the general Catalogue access service (influenced by SDSS CAS CASjobs project), based on original algorithms and open-source software. ... SAI MSU | ...

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TUI supports the following offsets: . Object Arc offset by a given amount on the sky (i.e. along the arc of a great circle). ... Arc offsets are useful for moving a different portion of your object or a different nearby object onto the boresight . ... Object Arc XY this is identical to an Object offset except that it has been rotated to align along the instrument x-y axes. ... This is just like the Calibration XY offset, except that it is typically cleared when you slew to a new object. ...

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• Primary mirror support