... Within the XMM pipeline it is necessary to make a decision a priori whether a given exposure in an observation should be passed through the normal ``scientific'' pipeline. ... This decision is based solely on information readily available from the ODF (via the OAL), for example instrument mode, filter wheel position (except RGS), exposure duration, etc. ... EPIC MOS or pn exposures which are not in a supported mode (see list below) . ... OM science user defined, EPIC M1 image, EPIC M1 image/fast, . ...

... Purpose: The purpose of this program is to monitor the long-term stability (time-scale: 1 year) of the sensitivity of ECH-A, ECH-B, and G140M. Description: This proposal defines a series of observations that will continue the long-term monitor of ECH-A, G140M, and ECH-B. ECH-A and G140M observations will be made both through the LSA and the SSA. ... Fraction of GO Programs Supported: All GHRS programs using ECH-A (11%), ECH-B (11%), and G140M (10%) in Cycles 4, 5, and 6. ...

... Space flight . ... Space camp . Space Hotel . ... The "Hydrospace" program is a unique complex of engineering facilities and is intended for training cosmonauts for their operations in outer space. ... The Neutral Buoyancy Laboratory includes : . ... A mock-up of the "Orlan-M" EVA-suit; . ... Air- and water supply systems complex; . ... The air- and- water supply systems are intended for provision of EVA- suit, diving equipment and diving decompression chamber with air and water. ...

... This is possible at modest cost due to the low moments of inertia of the telescope and enclosure. ... This same performance will be achieved in higher winds when the telescope enclosure is facing away from the wind, or by using wind screens. ... The telescope system (MILT) will be remotely operable with an on-site operator's assistance by an astronomer located at one of the ARC member institutions. ... Mean Wind Speed . ... Offsets > 10 deg: 1 arc sec rms max . ... 5 sec max, tracking to tracking . ...

... Scanning Fabry-Perot . ... This page is designed by A.V. Moiseev . ... The SCORPIO-2 project: . ... Afanasiev V.L. Moiseev A.V. "Scorpio on the 6 m Telescope: Current State and Perspectives for Spectroscopy of Galactic and Extragalactic Objects", 2011, BaltA, 20, 363 ( PDF ) . ... Moiseev A.V. 2002, "Reduction of the CCD-observations with scanning interferometer Fabry-Perot", Bull. ... Moiseev A.V., Egorov O.V., "Reduction of the CCD-observations obtained with the Fabry-Perot scanning interferometer...

... Driver ID: WWV_HEATH . ... This driver supports the Heath GC-1000 Most Accurate Clock, with RS232C Output Accessory. This is a WWV/WWVH receiver somewhat less robust than other supported receivers. ... Since the indicated precision is 100 ms, expect a host synchronized only to this thing to wander to and fro, occasionally being rudely stepped when the offset exceeds the default CLOCK_MAX of 128 ms. The internal DIPswitches should be set to operate at 1200 baud in MANUAL mode and the current year. ...

... For observations we selected all Case galaxies in the zone = - from the Case lists III, IV, V, VIII, XI, XII and XIII which were classified in the Case survey by some indication on presense of [O III ] 4959,5007 emission lines (vs - very strong, s - strong, m - medium, w - weak, w? - weak?) and which had not been observed yet. ... Аdditionally nine Markarian galaxies in the same sky region were observed in hope to have better completeness in picking up all probable BCGs. ...

... Science . ... Site Map . ... Science Users Information > Science Publications > Science Announcements > Upgrade of the Paranal Astronomical Site Monitor . ... Observing with ESO Telescopes . ... Data Handling and Products . ... Science Archive Facility . ... The ESO astronomical site monitor (ASM) system on Paranal has undergone a major overhaul. ... They are accessible via the Science Archive Facility Paranal ambient conditions page and a full description can be found via the help page . ...

It is a matter of common knowledge that in processes of genesis and evolution of many solar phenomena participate magnetic fields of sunspots. ... As a basis for formation of the database we take data on magnetic fields, collected by set of observatories during many years of observations. ... Section "Magnetic field data" contains data of magnetic field observation for separate sunspots, presented in standard text format (ASCII). ... Description of structure of these files is presented here . ...

... SMIS : Space Monitoring Information Support laboratory . Russia's Weather : State Meteorological Center Weather Forecast . Space Weather service : ACE real time solar wind data and simple geomagnetic activity forecast. ... World Fire Web : Space Research Institute (IKI) node . Sputnik : Joint project of SRC Planeta, Rosgidromet and Space Research Institute (IKI) . ... Today's Space Weather : Presented by the Space Environment Center . ... Back to the Space Research Institute Home Page ...

... They are concerned with Attitude Control System of the spacecraft, satellite visibility from tracking stations, limits on the satellite autonomous operations during the orbit, and needs for auxiliary operations with the spacecraft. ... Among the operational constraints the most important one is the number of programmed slews per orbit, which determines the maximum number of radio sources to be observed during one orbit. ... System temperature (K) . ... Progress of the RadioAstron Project in Pictures...

... Audible Indication of Any Network Condition. ... Label Configurations Standard Bindings NFPA110 GenSet Alarm and Status Annunciator The · · · · · · (A) The · · · · · · (A) The · · · (A) The · · · (A) following conditions are provided as High Battery Voltage (A) · Low Battery Voltage (A) · Generator Running (G) · Genset Supplying Load (G) · Pre- Low Oil Pressure (A) · Low Oil Pressure (R) · = Amber; (R) = Red; (G) = Green following conditions are provided as Check ...

The Australia Telescope Compact Array (ATCA) . Home page Team Galaxy Sample Observations Papers Projects Related Surveys Pipeline Meetings . Local Volume galaxies ( B. Koribalski) . The Local Volume HI Survey'' (LVHIS) is a project comprising deep HI line and 20-cm radio continuum observations for all nearby, gas-rich galaxies, supplemented by multi-wavelength data. ... Our aim is to study the formation and evolution of galaxies in the Local Universe. ...

. This diagram illustrates the relationship between the reference pixel and device pixels (called "dots" below). The image depicts a high resolution (large dot density) laser printer output on the left and a low resolution monitor screen on the right. For the laser printer, one square reference pixel is implemented by 16 dots. For the monitor screen, one square reference pixel is implemented by a single dot. Return to image.

MARS-96 . ROBOTIC SPACECRAFT MISSION TO MARS. Brief description . ... Scientific goals . Scheme of the mission . ... Description of . ... WIDE-ANGLE STEREOSCOPIC TV-CAMERA . ... Main scientific objectives: Global monitoring of time variations of the surface and atmosphere condition; in particular, cloud movements, changes due to dust storm, etc. ... Angular resolution (sec of arc/pxl) . ... Spatial resolution (m) from H-300 km . ... Angle of view (degree) . ... Convergence angle (degree) . ...

. Statistics of sunspot activity . The sunspot indices . My observations . NGDC's observations . The solar regions . Links . About authors . Russian pages . The solar regions . NOAA 11300's . NOAA 11200's . NOAA 11100's . NOAA 11000's . NOAA 10900's . NOAA 10800's . NOAA 10700's . NOAA 10600's . NOAA 10500's . NOAA 10400's . NOAA 10300's . NOAA 10200's . NOAA 10100's . NOAA 10000's . NOAA 09900's . NOAA 09800's . NOAA 09700's . NOAA 09600's . NOAA 09500's . NOAA 09400's . NOAA 09300's .

Next: Rotation Periods of ZAMS stars Previous: T Tauri Stars . ... The first attempts to directly measure periodic modulation of T Tauri stars occurred in the early 1980s. Rydgren & Vrba (1983) observed four PMS stars using photoelectric photometry over a period of seven consecutive photometric nights. ... Because the spot lifetime is much longer than the rotational period, the observed effect will be a modulation of the light from the star synchronously with the rotation period. ...

About us . ... Telescopes . ... Apart from the 6-meter telescope BTA two small telescopes are operative at SAO: the 1-m and 0.6-m telescopes, both manufactured by Carl Zeiss, Jena, are located near the BTA. ... These telescopes are used for adjusting the equipment and techniques of observations used at the BTA. ... The observational time allocation and also a brief description of the equipment of the 1-m telescope, which is used either permanently or mainly on this telescope, are presented below. ...

Next: Program use Up: Description of program searchdup Previous: Description of program searchdup . Parameter input is done with a graphic user interface. ... Input file: Name of the input catalog file. It has to be formatted, one record per source/observation, according to the format used in the Arcetri observations and source archives. ... Minimum number of observations per source Source with less than this number of independent observations are not included in the output file . ...

. Information for database users . Go to previous page . Description and abbreviations (minor planets) . Description and abbreviations (planets and satellites) . Information about observations . List of publications .