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1. mcfile
... This file contains the information about IB_TAIL and IB_AUR (AURORAL) magnetic conjugations as a function of the Universal time. The predicted magnetic conjugations correspond to the less then 5 deg relative geocentric angular distance of the two satellites magnetic footprints. ... the difference between two satellites corrected geomagnetic local times (see as well column 11) . ... the difference between two satellites corrected geomagnetic latitude (see as well column 12) . ... AnD (deg) . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/vprokhor/descr/mcfile.htm -- 5.1 Кб -- 12.05.1999
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/vprokhor/descr/mcfile.htm -- 5.1 Кб -- 12.05.1999
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2. http://www.ipa.nw.ru/conference/2002/sovet/PS/KESHIN.PS
... 8, ``Celestial Mechanics'', 2002 First results of GPS orbit determination with GRAPE package using a square--root information filter M. O. Keshin Institute of Applied Astronomy, St. Petersburg, Russia The zero--differenced carrier phase measurements contain the distance be­ tween the phase centres of receiver and transmitter antennas biased by unknown integer number of cycles (phase ambiguities). ... In the case of GPS the problem of solar radiation pressure modelling is of primary importance. ...
[ Текст ]  Ссылки http://www.ipa.nw.ru/conference/2002/sovet/PS/KESHIN.PS -- 28.3 Кб -- 19.08.2002
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3. http://www.apo.nmsu.edu/35m_operations/35m_manual/Instruments/CorMass/Files/cormass2.pro
pro cormass2,list ; ;procedure to pre-process CorMASS 'differenced' images to correct for reset ;voltage decay effects seen in NICMOS3 images. ... Sep '00 ; ; on_error,1 nl=numlines(list) ;find number of files print,'nl: ',nl files=strarr(nl) openr,lun,list,/get_lun readf,lun,files free_lun,lun for i=0,nl-1 do begin oldim=float(readfits(files[i],hdr)) d=size(oldim,/N_DIMENSIONS) if d GT 0 then begin magicsub2,oldim,procim sxaddhist,'Reset Decay Corrected w/ MagSub2',hdr,/PDU name=str_sep(files[i],'.' ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/35m_operations/35m_manual/Instruments/CorMass/Files/cormass2.pro -- 2.4 Кб -- 08.07.2004
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4. 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 . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/vprokhor/camp2/corcoord.htm -- 3.3 Кб -- 08.08.1997
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5. Natural Satellites Service. Apparent Encounters of the Tycho-2 Catalogue stars
Natural Satellites Service. ... Apparent Encounters . of the Tycho-2 Catalogue stars and the main natural planetary satellites . ... Suggestions . ... Here we present the precalculated circumstances of the apparent encounters of the stars of the Tycho-2 Catalogue with the main satellites of Saturn (S1-S8) for the period from November 2004 to February 2010, and with the Galilean satellites of Jupiter for the period from November 2004 to October 2010. ...
[ Сохраненная копия ]  Ссылки http://lnfm1.sai.msu.ru/neb/nss/SatStar/SatStarSugg.htm -- 4.4 Кб -- 14.12.2007
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6. SourceListFile
... The source-list file produced by omdetect contains a list of the positions of all the detected sources, the parameterizations of their shapes, their extracted count-rates, and corrected count-rateswhich contain some of the corrections that are needed to convert the raw rates to the rates that can be used to compute instrumental magnitutes. ... For example, a source with a bad pixel and lying on or close to a read-out streak would have bits 0 and 1 set and thus have a quality flag value of 3. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.0.0/doc/omdetect/node9.html -- 10.4 Кб -- 28.06.2006
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7. Container Widgets
... A child widget can then be added to this EventBox: gtk_container_add (GTK_CONTAINER (event_box), child_widget); . ... Resizing the window reveals varying amounts of the label . #include stdlib.h #include gtk / gtk .h int main( int argc, char *argv[] ) { GtkWidget * window ; GtkWidget * event_box ; GtkWidget * label ; gtk _init ( argc, argv); window = gtk _ window _new ( GTK _ WINDOW _TOPLEVEL); gtk _ window _set_title ( GTK _ WINDOW ( window ), Event Box ); g_signal_connect (G_OBJECT...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/~satr/GTK2/ch-containerwidgets.html -- 5.9 Кб -- 19.07.2002
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8. Differences Between QPOE Files and Image Arrays
Next: Other Types of Files Up: IRAF/PROS Files Previous: *.imh and *.qp Extensions . QPOE files are event lists. ... Image arrays are arrays of numbers representing total counts at each position - even if that count may be zero. ... Storing of images in the data directory . ... Filtering on QPOE files . On the command line, filters of the PROS type on QPOE files must be specified within quotes. e.g. im> imcopy "xdata$rp110590.qp[pi=2:10]" foo.imh # the input file # is rp90.imh . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node17.html -- 6.9 Кб -- 01.10.2012
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9. Index of /science/starburst/templates/fos_ghrs_spectra
... The spectra used in making the composite are in the "corrected" directory described below. column 1: rest wavelength in Angstroms column 2: average flux of the rectified corrected spectra column 3: median flux of the rectified corrected spectra In constructing the composite regions of geocoronal emission were masked in the input spectra. ... The files are in text format: column 1: restframe wavelength in Angstroms column 2: corrected flux in ergs/s/cm^2/Angstrom column 3: rectified corrected flux ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/starburst/templates/fos_ghrs_spectra/ -- 3.8 Кб -- 05.02.2013
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10. CHIANTI atomic database
The CHIANTI database consists of 4 primary ASCII files for each ion in the database. contains the energy levels in cm^(-1) It includes both experimental data and theoretical values of the levels energies. ... The 24 configuration model used to derive the transition probabilities in the ".wgfa" file, gave energy levels which were slightly different from the observed levels. ... contains the spline fits to the electron collision strengths scaled according to Burgess and Tully (1992). ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/chianti/chianti_4.01/database/fe/fe_12.html -- 6.9 Кб -- 02.12.2002
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11. Stellarium: Satellite Class Reference
Stellarium 0.12.3 . ... Classes . ... FileљStructure . ClassљList . ... Satellite Class Reference . A representation of a satellite in Earth orbit. More... #include < Satellite.hpp > . ... Thanks to operator<() overloading, container classes (QList, QMap, etc) with Satellite or SatelliteP objects can be sorted by satellite name/ID. ... The documentation for this class was generated from the following file: . home/aw/devel/stellarium/trunk/plugins/Satellites/src/ Satellite.hpp . ...
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/classSatellite.html -- 4.5 Кб -- 28.02.2014
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12. http://www.wdcb.ru/stp/data/cosmic.ray/Neutron_Monitors(minute_values)/C/2001C/2001CALG/REME5M.TXT
This directory contains Calgary Neutron Monitor Data at five minute resolution. Each file is a gzipped tar archive that contains files of uncorrected count rates and barometric pressures at five minute intervals for one year. A file named snm.calg.fmi.YYYY.tgz is an archive that holds five minute data for the year YYYY. ... So a file named cal01030.fmi contains five minute uncorrected data for year 2001 day 30 (which is Jan 30, 2001). ... A text file named note.txt is also usually present. ...