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1. East Siberian Center for the Earth's Ionosphere Research. Modelling, secondary
Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Although their determination is based on the scattering process model, independent check-ups by rocket experiments have shown their correctness in experimental applications. ... Ionospheric data analysis, especially during strong disturbances, cannot be without some other kinds of diagnostic tools. ... The lack of data has always been a challange in this case. ...
[ Сохраненная копия ]  Ссылки http://rp.iszf.irk.ru/esceir/isr/ismodelen.htm -- 5.9 Кб -- 04.06.2001
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2. User Parameters - Spectral-line Imaging CentralProcessor 0.11 documentation
... CentralProcessor 0.11 documentation . ... There are several steps involved in running the spectral-line imaging, with several optional pre-processing steps: . ... The gains solution from the continuum self-calibration can be applied to the spectral-line MS using ccalapply. The continuum can be subtracted from the spectral-line MS using ccontsubtract The continuum is represented by either the clean model from the continuum imaging, or ? ... Whether to do the spectral-line imaging . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/askapsoft/sdp/docs/current/BETApipelines/ScienceFieldSpectralLineImaging.html -- 22.5 Кб -- 12.04.2016
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3. Parameters
... Meta Index / Home Page This section documents the parameters recognized by this task (if any). ... boolean . ... false true . If startviewer is set to true imgdisplay attempts to establish a communication link between itself and an active Ds9 / SAOtng process upon invocation. ... If withreceive is set to true output from a running Ds9 / SAOtng process (resulting from a preceding execution of commands via withcommands / commands ) shall be collected in this parameter as a list of strings. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.0.0/doc/imgdisplay/node4.html -- 14.8 Кб -- 28.06.2006
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4. http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf
... Basic Observables: Zero-differenced phase and code ionosphere-free combinations of global GNSS network stations, corrected by P1-C1 satellite code biases (cc2noncc), daily observations with 30 seconds sampling rate Sites coordinates : IGb08 reference frame coordinates and velocities Displacements: solid tides, ocean loading, pole tide loading (IERS 2010) Geometric model : Receivers antennas eccentricities, absolute receiver and ...
[ Текст ]  Ссылки http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf -- 2427.5 Кб -- 30.11.2014
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5. http://www.mrao.cam.ac.uk/~kjbg1/lectures/lect1_1.pdf
... Luminosity (L) · · · · A source's luminosity is the power that it emits in radiation. ... NB Astronomers often say `flux' when they mean `flux density' · SI units are Wm-2Hz -1 -26 filter · Also used are Jy 10 Wm-2Hz -1 E= РРРF d dA dt Specific Intensity, Surface Brightness (I) · Specific intensity (or surface brightness) is the power received (or emitted) per unit area per unit frequency per unit solid angle. ч F at surface of a spherical source = I · · Specific intensity is independent of distance...
[ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~kjbg1/lectures/lect1_1.pdf -- 117.5 Кб -- 07.10.2002
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6. Other parameters of the evolutionary scenario
Next: Parameters of the starburst Up: The Model Previous: Initial parameters of compact . ... If the rate of accretion from one star to another is sufficiently high (e.g., the mass transfer occurs on a timescale a few times shorter than the thermal Kelvin-Helmholz time for the normal companion) or the compact object is engulfed by a giant companion, the common envelope (CE) stage of the binary evolution can set in (see Paczynski 1976; van den Heuvel 1983). ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~polar/html/publications/apj/node5.html -- 5.1 Кб -- 21.06.1996
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7. Line parameter measurements
Next: Results of follow-up spectroscopy Up: Data reduction Previous: Reduction of the Calar . In the final spectra, redshifts and line fluxes are measured within MIDAS, applying Gaussian fitting to the emission lines. To determine redshifts for individual galaxies, averages are taken over the prominent individual emission lines (mostly H , H , [O III ] 4959,5007 ?) The line [O II ] 3727 ? ... For all spectra, the individual emission line fluxes of the H , [N II ] 6548,6583 ? ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Laboratory/Publications/2000/HSSIII/node8.html -- 6.0 Кб -- 08.02.2000
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8. Parameters
Next: System configuration Up: How to use CONSTRICTOR Previous: Preparation of parameter file Contents . ... DayNumber: Even though this number is in the data, some packet headers have the wrong number and it makes it a whole lot easier to have the user check and enter this number correctly. ... CONSTRICTOR will add a multiple of 24 hours to the time tag when the day number changes. Remember to set the StopTime to, say, 48 hours if you use a DayNumber of one less than the actual day number. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~chummel/oyster/manual/node229.html -- 7.3 Кб -- 28.04.2015
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9. Introduction
Next: Image Formation Up: Improved Prescription Retrieval and Previous: Improved Prescription Retrieval and . Image restoration is the process of removing artifacts caused by telescope imperfections from images. ... As part of the ST ScI Image Restoration Project, and continuing under new NASA funding, we are exploring improved ways for determining telescope imperfections, and for using that information to compute accurate point spread functions (PSFs) for restoration. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/irw/proceedings/reddingd.dir/section3_1.html -- 7.1 Кб -- 18.04.1994
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10. Satellite Data Processing
Basics of magnetosphere satellite experiment. Main steps of data processing. Modern conception of Earth magnetosphere. ... Empirical models of the bow shock, magnetopause and neutral current sheet positions. Main principles of construction of empirical magnetospheric magnetic field models. ... Current systems in the Earth magnetosphere. Chapman- Ferraro current. ... Tsyganenko 1996 model and its application to satellite data processing. ... Basics of statistical data analysis. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/courses/met_obr_sup_dan_e.html -- 3.5 Кб -- 23.01.2004
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11. http://www.naic.edu/~astro/School/Talks/large_pdf/handson_ao6_2.pdf
Polarization the Central Calibration of Pixel of ALFA Hands-on Project AO-6 Outline Motivation Observational Setup Calibration Data Analysis Results Future W ork 1 M o ti v a ti o n Determine the flux and % polarization of 3C286 Determine instrumental polarization of ALFA beam zero without assumi ng source parameters Characterize i nstrumental polarization so that it can be removed i n future ...
[ Текст ]  Ссылки http://www.naic.edu/~astro/School/Talks/large_pdf/handson_ao6_2.pdf -- 344.5 Кб -- 17.07.2005
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