... 06jun11: testing the compressor monitor system on the telescope. 14apr11: testing the compressor monitor system in the lab . ... Around second 400 to 500 seconds, willie iguina openned the huffman box of the compressor monitor to get access to turn off the device. ... luis added some shielding to the devices in the huffman box (.pdf) and then remeasured the rfi on 15apr11. data was only measured up to 2500 MHz on this data with the huffman box closed. 902 probe: rfi below 100 MHz way down . ...

... Skalnatґ Pleso 43, 1 ­ 2, (2014) e Mini-MegaTORTORA ­ multichannel system for wide-field optical monitoring with high temp oral resolution V. Sasyuk1 , G. Beskin2 , S. Karp ov2 , S. Bondar3 , A. Perkov3 , E. Ivanov3 , E. Katkova3 and A. Shearer4 2 Kazan Federal University, Russia Special Astrophysical Observatory of Russian Academy of Sciences, Russia 3 Insttitute for Precise Instrumentation, Russia 4 National University of Ireland, Galway, Ireland Received: November 4, 2013; Accepted: ?? ...

HUBBLE SPACE TELESCOPE DAILY REPORT #1064 PERIOD COVERED: 0700 EST Daily Status Report as of 031/1200Z. 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed GHRS/2 5196 (GHRS SMOV Side 1 High Voltage Turn On) The High Resolution Spectrograph (Side One) was was turned on using its high voltage for early calibrations tests. ... 1.2 Completed WF/PC-2 5549 (GHRS Side 2 Dark Noise Monitor - Cycle 4) The WF/PC-2 was used to make internal tests for routine monitoring of detector dark noise. ...

To main of Laboratory . The research work and design of optical and optical-electronic devices are carries out by laboratory staff: . ... Lens: . ... In the layout 1 prism systems perform functions of dispersive element, corrector of aberrations, optical reducer. ... Spectral range 200 - 400 nm; . ... Back Forward . ... The main corrector's function are compensation of field aberrations of the main spherical mirror of a telescope (diameter of 600 mm, f'=1200 mm) and increase aperture ratio. ...

... European Remote Sensing Satellite (ERS-1) was launched on 17 July 1991, and the follow mission ERS-2 (with the same sensors and an Ozone monitoring instrument added) was launched on 21 April 1995. ... ERS-2 has a fixed repeat cycle of 35 days, and follows ERS-1 tracks with one day's delay. ... Swath width is 102.5 km (telemetered), spatial resolution is about 25x25 m. The Advanced SAR (ASAR) instrument is carried by ESA's ENVISAT satellite launched on 1 March 2002. ... Swath . ... Spatial Resolution...

... VLBI Schedule . ... Two different antenna are used for observing at ASKAP - AK07 has an L-band feed permanently installed while AK32 has an X-band feed installed. ... There are 3 main processes run for ASKAP observing. askap_drv is the main telescope control. It itself consists of a terminal based control process and a GUI. askap_drv must be running. VLBI scheduling is run from a process called "vlbi_drv", while the actual recording is via a command line process called px14_record. ...

... This document may be useful for those of you with S3-805 cards with GENDAC enhanced BIOS. ... It appears that the call to pfnPMSetmonitorTimings in svgadata.pmi is at the root of the problems faced by GENDAC owners. Warp's SVGA.EXE creates a SVGADATA.PMI that uses this call. The solution is to get a 2.1 version of SVGA.EXE and create another SVGADATA.PMI. ... Copy Warp's SVGA.EXE, the older SVGA.EXE and this document on a diskette or someplace accessible by DOS. ...

The study of energetic particles acceleration and transport within the magnetosphere and on its boundaries is the main goal of DOK-2 experiment on Auroral Probe in a frame of INTERBALL project. ... DOK-2 uses two pairs of energetic particle telescopes . ... This information is available only during the most informative Real Time mode of DOK-2. ... Full 56-57 channel spectra accumulated during time intervals from 10 s to 1464 s depending on a particle intensity. ... For this time interval: . ...