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21. http://xray.sai.msu.ru/~ivan/gmt/man/gmtmath.html
... By default, all columns except the "time" column is operated on, but this can be changed (see -C ). operand If operand can be opened as a file it will be read as an ASCII (or binary, see -bi ) table data file. ... I0 1 Modified Bessel function of A (1st kind, order 0). ... INV 1 1 / A. J0 1 Bessel function of A (1st kind, order 0). J1 1 Bessel function of A (1st kind, order 1). ... K1 1 Modified Bessel function of A (2nd kind, order 1). ... Y0 1 Bessel function of A (2nd kind, order 0). ...
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Ссылки http://xray.sai.msu.ru/~ivan/gmt/man/gmtmath.html -- 10.7 Кб -- 19.03.1999
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22. STScI NICMOS Software
Next: NICMOS Science Up: NICMOS Data Calibration and Previous: NICMOS Software at the . ... Reference File Tools . Image Analysis and Reduction . ... These include the tasks used in the STScI pipeline, tools to generate the reference files used by the calibration pipeline tasks, and general image analysis, manipulation, and arithmetic tasks. ... Calnica is used to apply instrumental calibrations to individual datasets, while calnicb is used to process associated sets of NICMOS images. ...
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Ссылки http://www.stecf.org/conferences/sardinia/node17.html -- 9.7 Кб -- 12.06.2006
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23. Description of SED models
... FTP access the basic models is here . ... Below, we put short descriptions of the used SED models for the photometric redshifts providing by the current server . ... The uniqueness of this model consists in expanding to the near IR (NIR) of Rocca-Volmerange and Guiderdoni's (1988) atlas of synthetic spectra with a revised stellar library, which includes parameters of cool stars. ... Homepage of the GISSEL model). ... Another model used earlier is the model of synthetic spectra of Poggianti (1997). ...
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Ссылки http://sed.sao.ru/sed_E_models.html -- 9.2 Кб -- 12.01.2005
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24. Astrophysics Group FIRST
... Astrophysics Group . ... FIRST . ... This site is an initiative by MRAO Cambridge to provide improved access for the UK to the images being produced from the FIRST survey. ... Note that a small image returned by this server will have different gridding and orientation from an image of corresponding position and size returned by the FIRST CUTOUT server at the main site. ... This site may evolve to provide more of the facilities available at the FIRST main site in due course. ...
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Ссылки http://www.mrao.cam.ac.uk/facilities/surveys/first/ -- 19.0 Кб -- 10.04.2016
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25. Description of algorithm
... The procedure of radiometer signal integration can be considered as a sort of reducing dimension of the initial sampling space, where the samples are the result of analog-to-digital conversion. ... The probability distribution of the signal and spikes is completely known. ... The quality of the considered algorithm could be also illustrated by Figure 2 . ... One could see the considered adaptive algorithm is preferable even by low degree of compression, because all spikes have been depressed. ...
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Ссылки http://mavr.sao.ru/hq/vch/Publications/Eng/html/NN/node2.html -- 11.5 Кб -- 28.12.2007
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/vch/Publications/Eng/html/NN/node2.html -- 11.5 Кб -- 11.09.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/vch/Publications/Eng/html/NN/node2.html -- 11.5 Кб -- 02.10.2012
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[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/vch/Publications/Eng/html/NN/node2.html -- 11.5 Кб -- 11.09.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/vch/Publications/Eng/html/NN/node2.html -- 11.5 Кб -- 02.10.2012
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26. ION Results Page
This page is a mirror of the ION SADS page available at http://sads.cnes.fr:8010 . Besides the information already available on this page, there you can browse the ION QuickLook images. ... The ION experiment flown on the Interball-Aurora mission performs simultaneous ion and electron measurements. Two mass spectrometers looking in opposing directions perpendicular to the satellite spin axis, which points toward the sun, measure ions in the mass and energy ranges 1-32 amu and ~ 0 to 14,000 eV. ...
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Ссылки http://www.iki.rssi.ru/auroral/ion.htm -- 5.1 Кб -- 23.04.1998
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/auroral/ion.htm -- 5.1 Кб -- 23.04.1998
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[ Сохраненная копия ] Ссылки http://www.cosmos.ru/auroral/ion.htm -- 5.1 Кб -- 23.04.1998
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27. http://www.cplire.ru/Lab144/iclp07.pdf
... The distinction of our approach is in that we unite the Actor Prolog concurrent ob ject-oriented logic language [ 1,2,3] with the Structural Analysis and Design Technique (SADT) diagrams to obtain new issues in the following areas: 1. ... Graphic user interface management. ... The individual blocks of visual user interface based on the SADT diagrams are implemented by using parallel processes of Actor Prolog. ... We applied the visual programming method for logic programming of Internet agents [4]. ...
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28. http://www.winer.org/Logs/NightLog-2014-11-24.txt
Date: 11/24/2014 Time:05:26 Moon Age: 1.8 Available Observing Hours: 12.9 Observer: Instrument: Operator: Cage: Lebofsky, Bell 90PrimeOne Trueblood PF hours lost to: weather: 2.0 telescope: 0.0 instrument: 0.0 computer: 0.0 Time Temp Humidity Wind Vel. Wind Dir. Seeing Open 18:30 37.8F 50% 15 N 1.9 Close 05:20 37.1F 15% 15 NE 1.8 _________________ Description ______________________ Most of the night, seeing >2", which severely limited our available targets. ...
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Ссылки http://www.winer.org/Logs/NightLog-2014-11-24.txt -- 1.8 Кб -- 02.12.2014
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29. API Help (ImageJ API)
... This API (Application Programming Interface) document has pages corresponding to the items in the navigation bar, described as follows. The Overview page is the front page of this API document and provides a list of all packages with a summary for each. ... Each package has a page that contains a list of its classes and interfaces, with a summary for each. ... Each of these pages has three sections consisting of a class/interface description, summary tables, and detailed member descriptions: . ...
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Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/help-doc.html -- 10.5 Кб -- 02.12.2010
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30. Journal "Peremennye Zvezdy"
Peremennye Zvezdy", . ... V348 Aql, USNO-B1.0 0904-0422027 . ... Meinunger (1966) classified it as an eclipsing binary with a period very close to 1 day, noting however that the period and derived minima times were uncertain due to the low variability amplitude. As of July 2011, the O C gateway (Paschke Brat 2006; Paschke 2009) lists, in addition to Meinunger's photographic data, 2 visual and 3 CCD times of minima from Paschke (1988, 1996, 2006), Stepan (1995), Br t et al. ... Meinunger (1966) . ...
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Ссылки http://www.astronet.ru/db/varstars/msg/1252756 -- 18.0 Кб -- 17.11.2011
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31. Description of database
GENERAL DESCRIPTION OF DATABASE . It is a matter of common knoledge, that solar magnetic fields and, in particular, magnetic fields of sunspots, play important role in many solar events. In Pulkovo observatory the long-term data set of daily observations of magnetic fields of solar sunspots was accumulated, which contains great potential for further researches in solar physics. ... Second section includes files containing sum data about magnetic fields for every observational day. ...
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Ссылки http://www.gao.spb.ru/database/mfbase.old/baseinfo.htm -- 5.7 Кб -- 21.05.2007
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32. Gemini NIFS Brief Description.
. NIFS overview . NIFS spectrograph . NIFS science . NIFS detector . NIFS integral-field unit . NIFS sensitivity . NIFS diffraction effects . NIRI legacy . Home * Brief Description * . Manuals * Performance Predictions * Picture Gallery * . Publications * Team Members * Internal Project Links * . Instrumentation Links * Gemini Project Links * Other IR Instruments
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Ссылки http://www.mso.anu.edu.au/nifs/description/index.shtml -- 4.6 Кб -- 01.10.2012
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33. pr-7
Magnetic field experiment on Vega - 1 and 2 spacecraft. ... Two spacecrafts, Vega-1 and Vega-2 have been launched aboard Proton rockets from Baykonour on 15 and 21 December 1984, respectively. ... During the cruise phase from Earth to Venus both Vega-1 and Vega-2 spacecrafts had one-axis orientation i.e. Bx of magnetometer was directed to the Sun, By and Bz axes were rotated around Bx-axis. ... Spacecraft position data are presented in HGI and SE systems. ... Vega-1 magnetic data for 1984 . ...
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Ссылки http://www.izmiran.rssi.ru/projects/PROGNOZ-MF/vega.htm -- 6.9 Кб -- 07.04.2008
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34. The NMW survey homepage
NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...
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35. Manual Page: htdigest - Apache HTTP Server
NAME htdigest - Create and update user authentication files SYNOPSIS htdigest [ - c ] passwdfile realm username DESCRIPTION htdigest is used to create and update the flat-files used to store usernames, realm and password for digest authentica- tion of HTTP users. Resources available from the httpd Apache web server can be restricted to just the users listed in the files created by htdigest. This manual page only lists the command line arguments. ... OPTIONS -c Create the passwdfile . ...
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Ссылки http://neptun.sai.msu.su/manual/programs/htdigest.html -- 3.6 Кб -- 15.10.2001
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36. Stellarium: StelLocationMgr Class Reference
Stellarium 0.12.3 . ... ClassљList . ... StelLocationMgr Class Reference . Manage the list of available location. ... locationForString (const QString &s, bool *ok=NULL) const . ... Get whether a location can be permanently added to the list of user locations The main constraint is that the small string must be unique. bool StelLocationMgr::deleteUserLocation . ... Return the StelLocation for a given string Can match location name, or coordinates. bool StelLocationMgr::saveUserLocation . ...
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Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/classStelLocationMgr.html -- 20.3 Кб -- 28.02.2014
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37. http://www.wdcb.ru/stp/data/solar.act/sunspot/sunspot.txt
RELATIVE SUNSPOT NUMBERS Description of Data from SGD Explanation of Data Reports: Relative Sunspot Numbers -- The relative sunspot number is an index of the activity of the entire visible disk of the Sun. ... The provisional daily Zurich relative sunspot numbers, Rz, were based upon observations made at Zurich and its two branch stations in Arosa and Locarno and communicated by M. Waldmeier of the Swiss Federal Observatory. ... This indicates the uncertainty above and below the predicted number. ...
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Ссылки http://www.wdcb.ru/stp/data/solar.act/sunspot/sunspot.txt -- 5.2 Кб -- 18.01.2010
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38. Diving in space suit ORLAN M at neutral buoyancy laboratory at space center.
... Space flight . ... Space camp . Space Hotel . ... The "Hydrospace" program is a unique complex of engineering facilities and is intended for training cosmonauts for their operations in outer space. ... The Neutral Buoyancy Laboratory includes : . ... A mock-up of the "Orlan-M" EVA-suit; . ... Air- and water supply systems complex; . ... The air- and- water supply systems are intended for provision of EVA- suit, diving equipment and diving decompression chamber with air and water. ...
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Ссылки http://www.atlasaerospace.net/eng/aqua-tech.htm -- 34.8 Кб -- 09.04.2016
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39. http://scan.sai.msu.ru/omc_converter/
. Please enter the lightcurve FITS file name: . Lightcurve file: . Please note, the output dates are Barycentric-corrected Julian Dates expressed in Terrestial Time - BJD(TT). A similar FITS-to-ASCII lightcurve converter is available for SuperWASP data. If you have questions, bug reports or suggestions how to improve this service, please fell free to contact the author (Kirill Sokolovsky) via e-mail: kirx[at]scan.sai.msu.ru .
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Ссылки http://scan.sai.msu.ru/omc_converter/ -- 2.6 Кб -- 14.01.2013
[ Сохраненная копия ] Ссылки http://saistud.sai.msu.ru/omc_converter/ -- 2.6 Кб -- 14.01.2013
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40. VISTA ETC - Exposure Time Calculator
... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...
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Ссылки http://www.vista.ac.uk/observing/etc/index.html -- 15.1 Кб -- 28.03.2013
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