Next: Site Up: Summary Report Previous: Summary Report Contents . In order to relate the phenological data with climate change, it is essential that a nearby meteorological station exists which can provide information on local environmental variables such as precipitation, temperature, sunshine and humidity. The Armagh Observatory, which has the longest climate record in Ireland and one of the longest in the UK, is therefore a prime location for such a garden. ...

... You are here: start €Ё lbaops €Ё observingnotes . ... VLBI Schedule . ... Observer's Wiki . ... lbaops:observingnotes . ... DAS . ... Disk loading . ... ATNF Machines (9 July 2008) . To run a VLBI experiment, a number of independent programs need to be run. This include a program to control the telescope and IF setup, controlling the DAS and the LBADR disk recorder. ... If starting the recorder late, or when changing disk partition during an experiment do not use the scheduled start. ...

... The previous example, Chapter 12, "Expanding Colored Squares Example," illustrates how to expand and contract the clipping region of a layer without changing the wrapping width of the layer. This example illustrates how to capture mouse events so that the user can make a layer's wrapping width wider or narrower by dragging the mouse. ... how to capture mouse events for a layer . how to change the wrapping width of a layer by using the load() function . ... Capturing Events for the Layer . ...

... Astronomical Observatory, Shevchenko Park, Odessa, 65014, . ... The XVI -th G. Gamow's Odessa Astronomical Summer Соnference-School, 14-20 August, 2016, Odessa, Ukraine . ... The XV -th G. Gamow's Odessa Astronomical Summer Соnference-School, 16-23 August, 2015, Odessa, Ukraine . ... The XIV -th G. Gamow's Odessa Astronomical Summer Соnference-School, 17-23 August, 2014, Odessa, Ukraine . ... The XIII -th G. Gamow's Odessa Astronomical Summer Соnference-School, 19-25 August, 2013, Odessa, Ukraine . ...

Ground Support of RadioAstron . Control and Tracking Stations . RadioAstron satellite control (command transmission, telemetry, orbit measurements) will be conducted from Evpatoria and Bear Lake control stations. ... Coarse orbit measurements will be carried out from control stations. Each measurement takes ten minutes. ... Orbit measurements at tracking stations give only radial component of spacecraft velocity but the measurements are going continuously during observing sessions. ...

... Observational Zoo of Binaries with Compact Stars . Evolutionary Scenarios of Binary Systems . ... Evolution of Magnetic Rotators . ... Mixing types of E-P-A binary systems with non-zero orbital . ... Binary Pulsar Diversity and High Neutron Star Birth Velocity . ... Ejectors in Massive Binary Systems . ... Other Candidates for Ejecting Stars in Binary Systems . ... Cosmic Rays and Evolution of Binary . ... Sky in Gravitational Waves . ... Gravitational Waves from Coalescing Compact Binary Stars . ...

... WSTLDREC - LOAD STRUCT FROM ASCII INPUT . ... The default is:/share/megs2_u1/wst/ . ... Previous Routine] [Next Routine] [List of Routines] NAME: wstrawinpday - read in 1 days worth of data from ascii file SYNTAX: n=wstrawinpday(yymmdd,bar,inpdir=inpdir) ARGS: yymmdd: int yymmdd of date for file (ast) inpdir : string input dir to read file. def: '/share/orion/' RETURNS: n: int number records input bar[n]: struct input data DESCRIPTION: Input a days worth of wst data from the daily raw: wst_yymmdd...

... Higgs, 1989; DRAO 1991. ... 12-13 RA (hours) 15-16 RA (min) 18-22 RA (sec) (XX.XX) 24-28 RA error (sec) (XX.XX) ( blank = unknown ) 30 Sign of declination 31-32 DEC (degrees) 34-35 DEC (arcmin) 37-40 DEC (arcsec) (XX.X) 42-45 DEC error (arcsec) (XX.X) ( blank = unknown ) 47 Epoch of coordinates (1=B1950, 2=J2000, 3= unknown ) 49 Type of position determination (1=rough estimate, 2=centroid, 3=peak, 4=fitted Gaussian, 5= unknown ) 51-56 Flux #1 ( variable format ) 58-62 Error in ...

Next: Imaging by an Optimizing Method . ... A big advantage of this numerical integrator is its stability: the error in the semi-major axis and the eccentricity depends only on the step size and does not grow with an increasing number of time steps. ... As the integration time increases, the numerical results become more contaminated by various errors. ... A new symplectic integrator produces no secular truncation errors in the actions of a Hamiltonian system. ...

... Acronyms and Abbreviations AMOS Advanced Mechanical and Optical Systems (UTM vendor) EIE FTT FLC ICD ISS European Industrial Engineering (UTE vendor) Fast Tip-Tilt First Light Camera Interface Control Document Interferometer Supervisory System NAS NMT NOT TBC TBD UT UTE UTM Narrow-field Acquisition System New Mexico Tech Nasmyth Optical ... Interface design description 2.5 FTT/NAS to ISS ICD This ICD describes the software interfaces of the FTT/NA system to the ISS. ...

... With this adjustment, the largest three-month range occurs in February-April and is 71 њF. The range for all year, still removing the January 1962 record low, is 88 њF. The expansion coefficient for aluminum alloy 6061 is 24.3 microns/m-њC while that for borosilicate glass E6 is 2.8 microns/m-њC. The expansion coefficient difference is 21.5 microns/m-њC. Combining this number with the scale factor equation from the previous section gives a coefficient of 0.207 mm/њC for primary motion. ...