Astronet Поиск по астрономическим сайтам English Russian
       
        Точная форма слов   О проекте   Сайты   Справка
Найдено документов: 20454 (73 сайтов) ---- Время поиска: 0.19сек.   

Пред. | 1 | 2 | 3 | 4 | След.

Показаны документы, содержащие фрагменты текста из документа
http://www.astro.spbu.ru/staff/afk/Teaching/Examples/F(x).htm.

21. Mid Scales Role
... ON THE ROLE OF LARGE-SCALE PLASMA IRREGULARITIES AT THE FINAL STAGE OF ANOMALOUS ABSOPTION DEVELOPING UNDER HF HEATING OF THE IONOSPHERE . ... Fig. ... With the aid of numerical statistical modeling based on multiple ray tracing it is shown that in presence of large-scale irregularities the reflected signal amplitude mean value is increased significantly. ... Dependence of the mean amplitude of the reflected from the ionosphere signal on the large-scale (10-50 km) electron density irregularity level...
[ Сохраненная копия ]  Ссылки http://ip.rsu.ru/~zabotin/posters/mid_sc/mid_sc.htm -- 11.1 Кб -- 02.02.2007
Похожие документы

22. IDL programs
FIRST SCREEN . Input files : image with wedges and image with spectrum (fits or tiff format). ... What to do : First of all you must fill in the region which the profiles should be taken from, by pressing "range for profiles" button. ... SECOND SCREEN . ... THIRD SCREEN . ... In the first screen you can change the size of the image by pressing "CHANGE SIZE" button. ... After pressing "Next profile" button, click to the same spectral lines in the same order as you did in the first profile. ...
[ Сохраненная копия ]  Ссылки http://lnfm1.sai.msu.ru/~kupry/SOFTWARE/fotocalib.html -- 5.5 Кб -- 01.10.2004
Похожие документы

23. Кольцо тереза авантюрин Носки унисекс 3PPK Value Cotton Crew, 3 пары SX4508-965
... Вставка: авантюрин. ... Кольца и перстни . ... Удобные носки унисекс Nike "3PPK Value Cotton Crew", изготовленные из высококачественного комбинированного материала, идеально подойдут вам. ... Носки имеют амортизационные элементы для комфорта и поддержки. ... Удлиненные носки оформлены контрастным логотипом Nike. В комплект входят три пары носков. ' title='Светодиодная лента Эра LS5050 60LED IP65 5m B 613955' border='0' align='left' width='120' style='margin-right: 20px;' hspace='7' vspace='5'/> . ...
[ Сохраненная копия ]  Ссылки http://astrokuban.info/astroku4113.html -- 18.2 Кб -- 14.02.2016
Похожие документы

24. SAI OCL Catalog Description
... Description . Catalog . ... In the Catalog, we publish equatorial (ЮБ 2000 , ЮД 2000 ) and galactic (l,b) coordinates of cluster centers derived as the position of overdensity in 2MASS catalog (Koposov et al. ... Distances, color-excesses and ages are the mean-square values calculated using all available evaluations from different color-magnitude diagrams. ... There are individual pages for every cluster where all available plots and parameters are published. ... 2002). ...
[ Сохраненная копия ]  Ссылки http://ocl.sai.msu.ru/description/ -- 5.9 Кб -- 09.04.2016
Похожие документы

25. http://selena.sai.msu.ru/Bus/Publications/m44_14_busarev_etal.pdf
... 13, Moscow 119992, Russian Federation, e-mail: busarev@sai.msu.ru; 2 Research Institute Crimean Astrophysical Observatory, p/o Nauchnyi, Crimea 334413, Ukraine, e-mail: prok@crao.crimea.ua Summary: We propose a combined method of astronomical investigations of small or distant planets incorporating registration of a set of integral spectra of an object and their frequency analysis. ... An application of the method is shown on example of asteroid 21 Lutetia. ... 6] Busarev V. V. (2002), Solar Sys. ...
[ Текст ]  Ссылки http://selena.sai.msu.ru/Bus/Publications/m44_14_busarev_etal.pdf -- 93.8 Кб -- 17.02.2009
Похожие документы

26. http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p153.pdf
Magnetic Stars, 2011, pp. 153 ­ 156 Ab out the Dep endence of the Rotation Velo city of CP Stars on the Magnetic Field Glagolevskij Yu. ... Based on the observational data of the average magnitudes of the surface magnetic field strength Bs for a number of chemically peculiar stars we investigate the dependence of the rotation period on the magnetic field. ... Now the periods of rotation P and the average values of the surface magnetic field Bs are known for more than 50 magnetic stars. ...
[ Текст ]  Ссылки http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p153.pdf -- 95.3 Кб -- 11.08.2011
[ Текст ]  Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p153.pdf -- 95.3 Кб -- 11.08.2011
Похожие документы

27. Description of the RadioAstron project, english version
Multi-Frequency Synthesis in K-band . The Multi-Frequency Synthesis (MFS) permits to realize a good quality imaging of the continuum radio sources in short time. ... The RadioAstron mission will operate one K-band circular polarized channel at fixed frequency 22,232 GHz. ... In general one K-band RadioAstron channel with fixed frequency will be unchanging and compatible with all the ground radio telescopes. ... Progress of the RadioAstron Project in Pictures . ...
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/RadioAstron/description/mfs_eng.htm -- 5.6 Кб -- 10.05.2008
Похожие документы
Еще в разделе: (Показать все результаты (>91) - www.asc.rssi.ru/ )

28. SAI CAS: Accessing SAI CAS from scripts
SAI VO . ... SAI CAS . ... Access . ... http://vo.astronet.ru/sai_cas/conesearch?RA= $RA &DEC= $DEC &SR= $radius &cat= $catalog &tab= $table &format= $format . http://vo.astronet.ru/sai_cas/conesearch?RA= $RA &DEC= $DEC &SR= $radius &cat= $catalog &tab= $table &format= $format &columns= $columns . http://vo.astronet.ru/sai_cas/conesearch?RA= $RA &DEC= $DEC &SR= $radius &cat= $catalog &tab= $table &format= $format &withdist= $withdist &NULLS= $nulls where . ... File to store the results . ...
[ Сохраненная копия ]  Ссылки http://vo.astronet.ru/cas/access.php -- 16.1 Кб -- 01.10.2012
Похожие документы

29. http://www.2dfquasar.org/Spec_Cat/fits_header.txt
... Equinox of object coordinates BJ = 18.87 / bJ magnitude UMBJ = -0.69 / u - bJ colour BJMR = 0.22 / bJ - r colour NOBS = 1 / Number of 2dF observations available IS_ BEST = 'TRUE ' / TRUE if this file contains the best 2dF observa DATEBEST= '24/09/00' / Date of best 2dF observation (DD/MM/YY) ID_ BEST = 'QSO ' / ID from best 2dF observation QUALBEST= 11 / Data quality flag from best 2dF observation Z_ ...
[ Сохраненная копия ]  Ссылки http://www.2dfquasar.org/Spec_Cat/fits_header.txt -- 5.1 Кб -- 03.03.2004
Похожие документы

30. Radioastrophysical Observatory ISTP RAS SB
... SHORT TERM PREDICTION OF POWER SOLAR FLARES FROM SSRT DATA . The algorithm for short term prediction of powerful solar flares, based on SSRT data, includes microwave emission characteristics in total and polarized flux, the structure of active region (AR) magnetic field at the photospheric level, and H a patrol data. ... During this period, 7 AR's crossed the solar disk, in which 20 flares of importance ? ... Data on AR's and magnetic fields were received from the Sayan observatory by teletype. ...
[ Сохраненная копия ]  Ссылки http://ssrt.iszf.irk.ru/forecastsru.shtml -- 25.5 Кб -- 27.02.2014
Похожие документы
Еще в разделе: (Показать все результаты (>12) - ssrt.iszf.irk.ru/ )

31. Catalogue explanation
CLEAN Map ps -- is a plot of the naturally weighted CLEAN image. The lowest contour levels (2 steps) on image is plotted at "clev" levels [Jy/beam], the peak brightness -- "max" values [Jy/beam]. The dashed contours indicate negative flux. The beam is shown in the bottom left corner of the images. The plot is in postscript format.
[ Сохраненная копия ]  Ссылки http://astra.prao.psn.ru/Molotov/Webpage/INFO/image_ps_explain.html -- 1.6 Кб -- 07.04.2005
Похожие документы
Еще в разделе: (Показать все результаты (>3) - astra.prao.psn.ru/ )

32. SPUTNIK, SST Adriatic Sea
... Sea Surface Temperature, restored from NOAA satellite data . You may use Java applet to view temperature maps in more detail. Using the applet, you can build "accumulated" temperature maps from selected data, get temperature values in any point and save the resulting image to your local disk. Date and time of the data . ... 6:01 (GMT) . ... 3.04.2016 . ... For information mail to: info@sputnik.infospace.ru . ...
[ Сохраненная копия ]  Ссылки http://sputnik.infospace.ru/noaa/engl/adriatic/sst.ssi -- 8.4 Кб -- 09.04.2016
Похожие документы

33. http://www.armaghplanet.com/pdf/AstroTopics/Beyond%20the%20Solar%20System/drake.pdf
... This is perhaps the most common question asked by visitors to the planetarium. ... This is known as the Drake Equation and reads as follows: N = R* fp ne fl fi fc L N is the number of communicating civilizations in the galaxy R* represents the average rate of star formation in the Milky Way Galaxy fp is the fraction of those stars that have planets around them ne is the number of planets per star that are capable of sustaining life fl is the fraction of planets in ne where life ...
[ Текст ]  Ссылки http://www.armaghplanet.com/pdf/AstroTopics/Beyond%20the%20Solar%20System/drake.pdf -- 93.5 Кб -- 20.09.2011
Похожие документы

34. AAL Homepage
... ARTICLE: The Adventurous Search For The Astronomical Unit . ... Kepler himself had suggested to use the rare occasions of Venus transiting (crossing) the solar disk to measure our distance to the planet. ... Due to the orbital inclination of Venus against the ecliptic of 3.5°, a Venus transit is so rare that it happens only at intervals of 121.5 years, 8 years, 105.5 years, 8 years and so on. ... Crabtree witnessing the transit of Venus 1639 . ... Transits of Venus - The Quest for the Solar Parallax...
[ Сохраненная копия ]  Ссылки http://www.aal.lu/SPECIAL_TOPIC/2/ -- 29.5 Кб -- 09.04.2016
Похожие документы
Еще в разделе: (Показать все результаты (>8) - www.aal.lu/ )

35. http://curl.sai.msu.ru/mass/download/doc/pmt_param_eng.pdf
... 2 Measurement of PMTs counting characteristics and selection of op erating p oint To select the operating point of the PMT, that is the optimal values of the high voltage supply and pulse discrimination threshold, the command run counting=hv value is provided in the program mass. ... Starting with the minimum voltage (say 550 V) run command run counting=550 for the measurement execution. ... It is recommended to take measurements for the set of values of 0.4, 0.6, 0.8, 1.0. ...
[ Текст ]  Ссылки http://curl.sai.msu.ru/mass/download/doc/pmt_param_eng.pdf -- 111.1 Кб -- 12.09.2015
Похожие документы

36. Accuracy of World positional CCD observations of the numbered minor planets
... For reliable estimation of the accuracy of asteroid CCD observations we usually consider from ten or more various NUMBERED MINOR PLANETS (NMPs) observed during several nigths per month (more then 50 positions). ... They can be considered as an indicator of accuracy of the CCD positional observations with given MPC code. ... For any NUMBERED minor planet the (O-C) values must be zero if the errors of observations and the errors of its theory are absent. ...
[ Сохраненная копия ]  Ссылки http://www.accuracy.puldb.ru/METHOD.HTM -- 21.2 Кб -- 05.12.2007
Похожие документы
Еще в разделе: (Показать все результаты (>100) - www.accuracy.puldb.ru/ )

37. http://site2010.sai.msu.ru/static/doc/DAfshari.pdf
Measurement of Sky Brightness at the Iranian National Observatory Davoud Afshari1 and Sadollah Nasiri1,2 1Physics Department, Zanjan University, Zanjan 45195-313, Iran; Institute for Advanced studies in Basic Science (IASBS), Zanjan 45195-1159, Iran; Measurement of light pollution 2 Introduction Among 34 candidate sites at the central part of the country, 5 sites namely Garkesh (in Kashan ), Kolahbarfi(in Kashan ), Deynava (in ... One of these is light pollution. ...
[ Текст ]  Ссылки http://site2010.sai.msu.ru/static/doc/DAfshari.pdf -- 472.0 Кб -- 27.10.2010
Похожие документы

38. VaST homepage
... VaST is a software tool for finding variable objects on a series of astronomical images. ... VaST performs object detection and aperture photometry using SExtractor on each image, cross-matches lists of detected stars, performs magnitude calibration with respect to the first (reference) image and constructs a lightcurve for each object. ... VaST FITS image viewer ./pgfv . ... Part I" PZP, vol. ... K. V. Sokolovsky, S. A. Korotkiy; "New Variable Stars Discovered by the NMW Survey" PZP, vol. ...
[ Сохраненная копия ]  Ссылки http://scan.sai.msu.ru/vast/ -- 122.2 Кб -- 21.02.2016
[ Сохраненная копия ]  Ссылки http://saistud.sai.msu.ru/poisk/ -- 122.2 Кб -- 21.02.2016
Похожие документы

39. http://cgm.iszf.irk.ru/irkt/info.htm
... GCR and SCR are primary cosmic rays. 10-15 years after the discovery of cosmic radiation (1919) there emerged two main avenues of investigation in the physics of cosmic rays (CR): 1) nuclear - elucidation of the origin of elementary particles and nuclear interactions; and 2) astrophysical (space physics) - solution of the problem related to the origin and variations (changes in intensity) of CR. ... Besides, the CR flux in interplanetary space is, strictly speaking, not isotropic. ...
[ Сохраненная копия ]  Ссылки http://cgm.iszf.irk.ru/irkt/info.htm -- 6.1 Кб -- 28.11.2002
Похожие документы

40. MPFS reduction routines HELP
... Next Routine] [List of Routines] NAME: ADD_HEADER PURPOSE: addition information from FITS-headers MPFS-frames DESCRIPTION: The function computes the total exposure, mean value zenit distance and modified FITS header CALLING SEQUENCE: Result =ADD_HEADER( headers ) CATEGORY: reduction MPFS-data INPUTS: Headers = String array FITS-headers from the MPFS data OUTPUTS: Header = String array containing the header from the FITS file. ... OPTIONAL INPUT KEYWORD PARAMETERS: BEFORE = Keyword string name. ...
[ Сохраненная копия ]  Ссылки http://sn.sai.msu.ru/~sil/mpfshelp/ -- 91.4 Кб -- 24.08.1999
Похожие документы
Еще в разделе: (Показать все результаты (>44) - sn.sai.msu.ru/ )

Пред. | 1 | 2 | 3 | 4 | След.

Rambler's Top100 RFBR Яндекс цитирования