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1. Corrected Geomagnetic Coordinates
... 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] ) . ...
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Ссылки http://www.iki.rssi.ru/vprokhor/descr/corcoord.htm -- 4.9 Кб -- 12.05.1999
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/vprokhor/descr/corcoord.htm -- 4.9 Кб -- 12.05.1999
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[ Сохраненная копия ] Ссылки http://www.cosmos.ru/vprokhor/descr/corcoord.htm -- 4.9 Кб -- 12.05.1999
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2. Mod-8 corrected image file
. 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
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Ссылки http://xmm.vilspa.esa.es/sas/7.1.0/doc/omichain/node17.html -- 3.5 Кб -- 09.07.2007
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3. ESO - Integration Cryo-vacuum
... 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...
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Ссылки http://www.eso.org/sci/facilities/develop/integration.html -- 27.0 Кб -- 10.04.2016
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4. Error in corrected times with odelaytime
... 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. ...
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Ссылки http://www.stsci.edu/hst/stis/documents/newsletters/full_stories/0106_odelaytime.html -- 13.7 Кб -- 12.04.2016
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5. Illumination Corrected Flat Fields
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. ...
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Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node59.html -- 3.3 Кб -- 23.02.1996
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6. Errors associated with reducing filterbank data
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. ...
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Ссылки http://www.atnf.csiro.au/people/pulsar/reduce/fbtime/errors.html -- 3.0 Кб -- 24.12.2007
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7. Corrected Geomagnetic Coordinates
... 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 . ...
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Ссылки http://www.iki.rssi.ru/vprokhor/camp2/corcoord.htm -- 3.3 Кб -- 08.08.1997
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8. http://www.cplire.ru/html/lab234/pubs/2007_08.pdf
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. ...
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Ссылки http://www.cplire.ru/html/lab234/pubs/2007_08.pdf -- 930.4 Кб -- 25.01.2008
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9. Moore Observatory Remote/Robotic Telescope
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 . ...
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Ссылки http://www.astro.louisville.edu/moore/cdk20/ -- 4.6 Кб -- 17.03.2013
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10. http://www.mrao.cam.ac.uk/~dag/UVFXT/ReadMe.txt
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 ...
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Ссылки http://www.mrao.cam.ac.uk/~dag/UVFXT/ReadMe.txt -- 2.6 Кб -- 11.04.2007
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11. Procedures for Data Reduction
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. ...
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Ссылки http://www.arcetri.astro.it/irlab/instr/longsp/doc/proc_dr.html -- 4.7 Кб -- 16.02.2000
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12. first light daytime
... 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 . ...
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Ссылки http://www.naic.edu/~phil/hardware/xmiterhf/firstlight_day_150618.html -- 24.0 Кб -- 26.06.2015
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13. Rainfall in Eugene Oregon
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 . ...
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Ссылки http://zebu.uoregon.edu/raining.html -- 7.4 Кб -- 10.02.2000
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14. A New PROS Task for Calculating HRI Source Intensities or Upper Limits
... 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. ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/chenj.html -- 11.4 Кб -- 03.11.2000
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15. http://www.mso.anu.edu.au/gsaoi/gallery/rsaa/pics/brochure.pdf
Telescope Tip-Tilt Secondary Mirror The tip-tilt secondary mirror on the ANU 2.3 m telescope · Measures and adjusts image position at 30 Hz · Corrects image blur produced by turbulence in the Earth's atmosphere · Both the tip-tilt secondary mirror and the 2.3 m telescope were designed and constructed by RSAA ...
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Ссылки http://www.mso.anu.edu.au/gsaoi/gallery/rsaa/pics/brochure.pdf -- 1391.8 Кб -- 26.11.2002
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16. The AstroStat Slog Blog Archive my first AAS. VI. Normalization
... Archives . ... One realization of mine during the meeting was related to a cultural difference; therefore, there is no relation to any presentations during the 212th AAS in this post. ... I cannot cover all perspectives from both disciplines but I think there are two distinct fashions in practicing normalization. $$\frac{1}{N(\theta)}\int_{\Omega} f(x;\theta)dx=1$$ . ... This is my last posting on my first AAS . Tags: AAS , measure , measure theory , normalization , PDF , pmf . ... Chandra Blog . ...
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Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2008/my-first-aas-normalization/index.html -- 22.6 Кб -- 01.03.2014
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17. A Method of Integrating
Next: Introduction . ... A spike immunity method of digital integrating radiometer signals in the jamming environment is described. ... The purpose of the method is real-time signal processing, and the basic is an alternative selection of the least offset signal estimation using nonparametric "Nearest Neighbor" rule. ... The additive spike-like jam makes the "tails" of the distribution "heavier" which leads to different offsets for linear and rank mean estimation on the integrating interval. ...
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Ссылки http://mavr.sao.ru/hq/vch/Publications/Eng/html/NN/NN.html -- 3.5 Кб -- 28.12.2007
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/vch/Publications/Eng/html/NN/NN.html -- 3.5 Кб -- 11.09.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/vch/Publications/Eng/html/NN/NN.html -- 3.5 Кб -- 02.10.2012
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[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/vch/Publications/Eng/html/NN/NN.html -- 3.5 Кб -- 02.10.2012
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18. Astro-Art Fun at Windmill Integrated Primary School, Dungannon | International
... The Story of the Christmas Star continues in Northern Ireland: on Friday 11 December 2009, at the Windmill Integrated Primary School in Dungannon. During the UNAWE Astro-Art Fun workshops, held by Miruna Popescu from Armagh Observatory, the children have listened to the story and then made their own interpretation of the story on the individually designed Christmas cards and creative paintings. ... International Year of Astronomy, Ireland National Node . ...
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Ссылки http://star.arm.ac.uk/scholars/iya/gallery/local_events/astro-art_fun_at_windmill_ps/ -- 12.0 Кб -- 31.12.2009
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19. http://www.wdcb.ru/stp/data/cosmic.ray/Muon_Telesc(hourly_values)/U/2002U/2002MOSE/0201MOSE.C0U
... 5883 5949 5897 5970 5938 5879 5967 5969 5909 5984 5939 5920 5990 5949 5863 5898 6004 6023 5944 5956 5946 5968 5943 5885 0201 2. ... 5983 5976 5966 5909 5970 5955 5917 5961 5942 6004 5989 5963 5946 6002 6017 5940 5932 5880 5932 5960 5971 5955 5907 5905 0201 4. 5992 5905 5904 5905 5983 5949 5921 5929 5927 5939 5944 6033 6009 5882 5956 5915 5953 5992 5892 5983 5952 5996 6019 5952 0201 5. ...
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Ссылки http://www.wdcb.ru/stp/data/cosmic.ray/Muon_Telesc(hourly_values)/U/2002U/2002MOSE/0201MOSE.C0U -- 2.4 Кб -- 02.11.2005
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20. VISTA Integration Time DIT Recommendations
... Appropriate values of DIT the integration time (DIT secs) for each individual integration, are lmited by various considerations. N.B. Ndit individual Integration s each of DIT secs are coadded to form a single Exposure of time Ndit*DIT]. The recommended minimum DIT is one sec (the minimum possible exposure time) or the value at which the noise becomes sky (rather than detector) limited. ... The recommended maximum DIT is such as to keep the detector wells less than half full. ... 40 sec . ...
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Ссылки http://www.vista.ac.uk/observing/dit.htm -- 10.6 Кб -- 24.10.2012
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