... It consists of two energy-angle analyzers EA-2 and EA-3 for low energy particles, and two identical oppositely directed time-of-flight (TOF) analyzers EM-1-1 and EM-1-2 for high energies. ... Analyzers of low energy charged particles (EA-2 and EA-3). ... The instruments allow to measure simultaneously in eight angular sectors evenly distributed in the angle 2 perpendicular to the satellite rotation axis, and sequentially in 7 energy intervals for each angular sector. ... Interval . ...

STScI . ... You can install this with easy_install or pip. ... If you will be installing on Linux or Macintosh, you also need pip and the compiler packages for your system. ... To install stsci_python, type these commands into a cmd window: c:\python27\Scripts\easy_install stsci.distutils . ... STSCI_PYTHON is now distributed as several separate packages, so that it can more readily fit into the pypi/pip/easy_install ecosystem. ... On Linux or Macintosh, use this command: pip install --download . ...

... JavaScript 1.1 Plugin objects are predefined JavaScript objects that you access through the navigator.plugins array. A Plugin object is a plug-in installed on the client. ... For example, the following code displays the type and description properties of the first Plugin object's first MimeType object. myPlugin=navigator.plugins[0] . ... Description . ... The following code assigns shorthand variables for the predefined LiveAudio properties. var myPluginName = navigator.plugins["LiveAudio"].name . ...

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. ...

... You are here: start €Ё difx €Ё documentation . ... Other useful collections of information . ... If you have not already, please join the DiFX-Users mailing list - to do this, go to https://listmgr.nrao.edu/mailman/listinfo/difx-users and sign up. ... The (now-defunct) forum on the old DiFX-users Google Groups page ( https://groups.google.com/forum/#!forum/difx-users ) might also have useful information, so feel free to swing past there and search old threads for answers to questions you might have....

... Meta Index / Home Page / Description . ... This can be set by the user via the parameter device . The default value of device is /XS (Xserver), but alternative outputs (depending on what drivers have been installed with PGPLOT) can be used, for example /XW for x-windows, /GIF, /JPEG, /PS for Postscript, and /CPS for Colour Postscript. ... Either a colour-coded image or a contour map image can be produced, depending on the value of imagestyle . ... Note that 0 is not a valid colour map index. ...

Description and Technical Details . In 1980s two medium-size horizontal solar telescopes 50/35000 cm with large spectrographs Czerny-Turner made by Carl Zeiss Jena were installed in the Ondњejov observatory. The Czerny-Turner-spectrographs in the Ondњejov observatory called HSFA1 and HSFA2 according to the German name Horizontal-Sonnen-Forschungs-Anlage ("horizontal device for solar research") have been explored for more than two decades. ... Diffraction grating - Richardson, Spectra-Physics . ...

Gain curve description, location, and code to evaluate the curves. ... Data taken mar03 to feb05. Gain curve installed 28feb05. ... Data taken mar05 . ... Data taken Mar03 thru sep03 Installed 02nov03. ... This is after the new horn was installed. ... Data taken 27aug02 thru sep02: This gain curve was made after the lbn horn focus was moved on 27aug02. ... The cband gain curve was taken from data 28aug02 thru 30nov02. ... Calibration data from mar03 thru sep03 was used to compute gain curves. ...

RTT150 . ... The primary mirror 1 reflects light to the secondary mirror 2 which sends the converging beam of light to the system of four flat mirrors 3, 4, 5 and 6. That allows the beam of light to leave the telescope strictly along its polar axis and be collected in Coude focus. ... That's why at any tube position (for any rotation along the declination axis) beam of light parallel to the principal axis after reflection on mirror 3 follows the direction of declination axis. ...

... Telescopes . ... Method "Spectroscopy with the Main Stellar Spectrograph (MSS) of the BTA" . ... The MSS of the 6-m BTA telescope is a long-slit spectrograph, stationary installed in the rack of the Nasmyth-2 focus (Vasiliev et al. ... Design, engineering and manufacturing of the spectrograph were carried out in parallel with the creation of the BTA telescope. ... Panchuk V.E., SAO Preprint ? ... BTA telescope. ... The main stellar spectrograph, Leningrad: LOMO (1974) (in Russian). ...

dfos = Data Flow Operations System, the common tool set for DFO . ... dfos tools . ... clMonitor.html, exported to http://qcweb.hq.eso.org/CLUSTER/monitor . ... The clMonitor gives an overview of the currently condor activity (nodes executing condor jobs) and the pending queue. ... idle | ... busy' indicates that condor currently executes a job on that node; 'idle' means no current condor job; 'reserved/not available' means the node is not configured for condor jobs, or is currently not available. ...