... 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-1.51) [xmmsas_20080701_1801-8.0.0] . 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 -- 2008-07-02

... 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. ...

... 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 . ...

... Science . ... Science Users Information > Data Handling and Products > Data Reduction FAQ > How good is HAWKI astrometry and how are PSF variations corrected? ... Science Users Information . Observing Facilities . ... Paranal Facilities . La Silla Facilities . ... Future Facilities and Development . ... Observing with ESO Telescopes . ... Science Software . ... Science Data Products Forum . ... Science Archive Facility . ... ESO Data . ... ESO Data Access Policy . ... ESO Science Newsletter . ...

... Execute) Back Status Jacks Limits # ListCtrl $ Caption =Jack Limits: $ ColumnName0 = Name $ ColumnName1 =Status $ StructName1 =Limits.Actual Back Drive Status # ListCtrl $ Caption =Drive Status: $ ColumnName0 = Name $ ColumnName1 =Status $ StructName1 =Jacks Alarms.Actual Back Positions # ListCtrl $ Caption =Jack Positions: $ ColumnName0 = Name $ ColumnName1 =Position $ ...

Institute of solar-terrestrial physics Russian Academy of Sciences Siberian Branch IRKUTSK 33, P.O.Box 291, 664033 RUSSIA IRKUTSK ( IRK3 ), 6 NM64 NEUTRON MONITOR, PRESSURE CORRECTED Altitude 3000 M Mean= 3096.6 August 2007 Geographic Coordinates 51.29 100.55 Rc(1965)= 3.64 GV; SF= 512 Pressure Coefficient= -0.720 %/mb Corrected to 715 mb Standard Pressure Comment: 1.000 3069 3076 3078 3081 3095 3117 3107 3099 3090 3090 3094 ...

... Classes . ... Class List . ... casa . casa::MSSelectionKeywords . ... Static Public Member Functions | ... DATA , . ... The fields in the MS for which selection and range operations are defined. ... the range of visibility amplitude . ... casa::MSSelectionKeywords::MSSelectionKeywords . ... This class is purely static, no instances are allowed. casa::MSSelectionKeywords::MSSelectionKeywords . ... static Field casa::MSSelectionKeywords::field . ... static void casa::MSSelectionKeywords::initMap . ...

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 . ...

... for Cosmic Ray Observation is situated in Irkutsk (Russia). ... Real-time (preliminary) cosmic ray data in Irkutsk . ... Online Cosmic Ray and Atmospheric Pressure Data Base . ... Real-time data Uncorrected for pressure (Resolution 1 hour - 1 year) -- since 05.2001 . Real-time data Corrected for pressure (Resolution 1 min - 1 year) --- since 09.2001 . Resolution 1 hour - 1 year) --- since 06.2001 . Final data Corrected for pressure (Resolution 1 hour - 1 year) --- From 01.1975 To 07.2004 . ...

ALMA | ... In this section, we explain why we need to correct phase fluctuations and ALMA's strategy to do this. Rapid fluctuations will be corrected with water vapour radiometers (WVRs). The Cavendish Astrophysics Group was also a leading contributor to the ALMA prototype WVRs, which were put through their paces in tests at the Submillimeter Array (SMA). ... The Cavendish Astrophysics Group in partnership with the Onsala Space Observatory built two prototype WVRs for the ALMA project. ...

In 1995 Eugene set an annual rainfall record by recording, officially, 65.56 inches of rain. ... The mean annual rainfall for Eugene from the 25 year period 1970-1994 was 51.5 inches with a dispersion of 8 inches. ... Wettest Years: . ... Below are the official NWS corrected rain totals for the year 1996. Although these are now "official", I go on record here by saying there is no way I believe that Eugene, Oregon received 101 inches of rain in 1996. ... January: Old = 14.74; corrected = 14.48 . ...

... FIX: Download corrected routines line_chianti.pro , popsol.pro , and nenh.pro and regenerate the CHIANTI database (or download) . NOTE: all tar files in the distribution have been updated. ... Updated all .pro files, include many enhancements and some minor bug fixes. ... 2001 Dec 07: . ... FIX: the files have been updated to correct for this. download new versions of rd_line.pro , fold_ioneq.pro , and rd_ioneq.pro . ... FIX: Copy corrected routine and replace . ... Fixed in all tar files. ...

... Stellar magnitudes, provided by observations in an optical band, are reduced to the units of erg/cm /s as follows: . ... Table: `Zero-points', central wavelengths, and effective widths of optical bands (Zombeck's Handbook, 1990). - the corrected value (the handbook value is given in parentheses). ... We have achieved coincidence between theoretical values by Bochkarev et al (1991) and ours, obtained with rectangular shapes of transmission band of optical filters. ... 1991, V. 1, P. 41. ...

. Northern JHK Standard Stars for Array Detectors . L.K. Hunt 1 , F. Mannucci 1 , . L. Testi 2 , S. Migliorini 2 , R.M. Stanga 2 , . C. Baffa 3 , F. Lisi 3 and L. Vanzi 3 . 1 CAISMI- CNR, Firenze . 2 Universita' di Firenze . 3 Osservatorio Astrofisico di Arcetri . published in AJ 115, 2594 (1998) . Paper text (postscript) . Erratum . Magnitude table (postscript) CORRECTED . Finding charts (postscript) CORRECTED . Magnitude table (ascii) CORRECTED

Here is one CCD image of the SN. ST7 image format. Dark and flat corrected, Mar 19,1998 at.01.11 UT, yellow filter, temp -20c, 600s track and accumulate exposure (20x30s). The telescope used is 150/2063mm refractor. ... The next image was taken at 29.3.1998 01.27 UT, CCD ST-7, 600 s. Track and Accumulate exposure (15x40s.), no filter, dark and flat corrected, temp -20c, telescope used 2063/152 refractor. ... Back to Supernovae in NGC and IC galaxies . Back to Supernova 1998S images . ...

... Team . ... The main goal of observations of GRB host galaxies is accumulation of statistics of their spectroscopic and photometric properties. ... The Hubble diagram for 22 GRB host galaxies with known magnitudes and redshifts (GRB 970228, GRB 970508, GRB 970828, GRB 971214, GRB 980613, GRB 980703, GRB 990123, GRB 990510, GRB 990712, GRB 9912008, GRB 991216, GRB 000131, GRB 000210, GRB 000301C, GRB 000418, GRB 000911, GRB 000926, GRB 001109, GRB 010222, GRB 010921, GRB 011121 and GRB011211). ... 600...

The following is a corrected version of Sea Of Sin which should replace the current one at ftp.uwp.edu:/pub/music/lyrics/d/depeche.mode/ sea _of_ sin Previous version by Anson Mayers, corrected version by Ryan Watkins vamp@csulb.edu) and the Depeche Mode Mailing List. ========================================================================== @song @ Sea of Sin -Depeche Mode, World in my Eyes Single Sea of Sin ...

... Next: The PROS Big Up: Software Systems Previous: Data Reduction Software . ... The srcinten task provides PROS users with a tool to compute count rates for point sources in the ROSAT High Resolution Imager (HRI). ... Corrected upper limits are cited at locations where the count rate falls below the source detection threshold. ... Srcinten is a new PROS task that computes and applies the above correction factors to the net counts in a user-specified aperture. ...