... Step 1: The magnetic field line tracing from the satellite position up to magnetic equatorial plane using IGRF magnetic field model. Step 2: Tracing back from the point (produced on the Step 1) to the Ionosphere (by using only dipole magnetic field) . ... The magnetic field line tracing from the satellite position up to the Ionosphere (the stop trace altitude 110 km) using Main (dipole) + Extraterrestrial magnetic field model (for example, Tsyganenko [1987], or [1989], or [1990] ) . ...

. XMM-Newton Science Analysis System . omichain (omichain-1.50) [xmmsas_20070708_1801-7.1.0] . Meta Index / Home Page / PPS Product Files Ommodmap produces a mod-8 corrected image from the intermediate image produced by omprep . Mod-8 corrected image produced by ommodmap - eg P0123920101OMS006IMAGE_1000.FIT or P0135720601OMS017FIMAG_V000.FIT The latter will be produced if omcomb has run on engineering-2 data. XMM-Newton SOC/SSC -- 2007-07-09

... Science Users Information > Observing Facilities > Instrumentation Development > Integration Cryo-Vacuum . ... Integration Cryo-Vacuum . ... MAD . ... Semented Mirror . ... Paranal Instruments . ... ESO Departments . ... July 2010 . ... October 2008 . ... Jan 2008 . ... Our department has been involved for many years in the first generation VLT instruments. ... MAD first MCAO ever . ... This visitor instrument was fully integrated uder the responsibility of the integration and cryo-vacuum department...

... HST . Error in corrected times with odelaytime . ... Missions . ... Data . ... Future Missions and . ... HST Overview . Overview . ... Cycle 24 Announcement . ... Retrieving HST Data . ... Error in "corrected times" using odelaytime with de200.fits . ... This causes an error in the barycentric correction to the time stamps, when using "odelaytime" with the STIS timetag data. ... We are fixing the header in the de200.fits so that 'odelaytime' will work correctly in the next release of STSDAS. ...

Next: Fringe correction Up: Special Processing Options Previous: Sky Illumination Corrected . A third method to account for illumination problems in the flat fields is to remove the large scale pattern from the flat field itself. This is useful if there are no reasonable blank sky calibration frames and the astronomical exposures are evenly illuminated but the flat fields are not. This is done by smoothing the flat field frames instead of blank sky frames. ...

About the only thing that can go wrong is not having the pulsar details correct in the catalogue OR not integrating for long enough. ... You can check what the catalogue thinks it knows about the pulsar by using psrinfo and typing . ... NSUB: - Number of frequency sub-bands . ... Note if you are reducing this data at Parkes you will have to copy psrcat.unformatted back up to $PSRHOME/soft/psrinfo at Parkes before rerunning tarchfb_driver. Back to the Filterbank data reduction page. ...

... Step 1: The Footprint position calculation by the magnetic field line tracing from the satellite position up to the Ionosphere by using IGRF + Tsyganenko [1987] magnetic field model (the stop trace altitude 110 km). Step 2: Tracing back from the Footprint (produced on the Step 1) to the dipole equatorial plane (by using only IGRF magnetic field model up to the geocentric distance 8 RE and dipole field model after this distance). ... Back to the description . ...

Integration and performance of the flight configuration SIR on TELIS P. Yagoubov1, G. de Lange1, A. de Lange, M. Romanini, R. Hoogeveen1, V. Koshelets2, G. Wagner3, M. Birk 1Nation 3 al Institute for ... Netherlands 2Institute of Radio Engineering and Electronics, IREE, Russia 3Institute for Remote Sensing Technology, DLR, Germany Abstract TELIS (Terahertz and submm Limb Sounder) is a cooperation between European institutes, DLR, RAL and SRON, to build a three- ... LO frequency 624.93 GHz. ...

The Planewave Instruments 20-inch (0.5-meter) f/6.8 corrected Dall-Kirkham telescope at Moore Observatory in Kentucky and its identical companion at Mt. ... The CDK20 North at Moore Observatory has been our primary platform for developing technology for remote and robotic operation in the Shared Skies program. ... g'r'z'i' filter wheel . ... Axis quad video server to send realtime video to the remote observer . ... Telescope monitor camera in the dome also on the video server . ...

UVFXT (to fix timestamps on GMRT uv data files within AIPS) =========================================================== To correct GMRT visibilites with timestamps near the beginning of the integration period, instead of middle. For example, for 16.9 s integrations, move timestamps on all uv data points forward by 7.4 s, (i.e. to centre of 16.9 s from the centre of the initial 2.1 s integration), and rotate u,v,w coordinates forward. ... Dave Green (dag@mrao.cam.ac.uk) -- MRAO -- 2007 April 11th ...

The main steps in the reduction of NIR spectroscopic data are flat-field correction, subtraction of sky emission, wavelength calibration, correction for telluric absorption and correction for optical system plus detector efficency. ... Sky subtracted frames are corrected computing analitically the tilt angle from the instrumental calibration parameters or directly measuring it from the data. ... The same procedures are applied to the reference stars frames to obtain the calibration spectra. ...

... total pwr in range vs ipp images . ... pol1 is the pol we started with. ... I was trying to write these times down as they happened. looking at some of the total power plots, it looks like some of the times were recorded were not correct (signal appears when hf off). ... To see when things happened, i made images of total pwr (in rang) vs time for each data file . ... The title of each image contains the start time (ast) as well as the state of hf xmiter when the file started. 5 sigma images . ...