Astronet Поиск по астрономическим сайтам English Russian
       
        Точная форма слов   О проекте   Сайты   Справка
Найдено документов: 36950 (99 сайтов) ---- Время поиска: 0.07сек.   

1 | 2 | 3 | 4 | 5 | След.

Показаны документы, содержащие фрагменты текста из документа
http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/arlines.redcuar.

1. The Water Vapor Channel
Astronomy Picture of the Day . ... 12.10.1996 . ... NASA/GSFC ) and The GOES Project Explanation: What alien planet's bizarre landscape lurks below these fiery-looking clouds? It's only Planet Earth , of course -- as seen on the Water Vapor Channel. Hourly, images like this one (shown in false color) are brought to you by the orbiting GOES 8 satellite's multi-channel imager . ... Bright regions correspond to high concentrations of water vapor while dark spots are relatively dry areas. ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/1161647 -- 12.9 Кб -- 23.04.2003
Похожие документы
Еще в разделе: (Показать все результаты (>6584) - www.astronet.ru/ )

2. Massaging Steps Performed by UVREAD - UVSET
... Object . ... data . channel . ... As mentioned above, the uvread routine can perform, at the programmers request, extra processing steps on the visibility data. ... If the original channels are numbers from 1 to , then, by using type='channel' , uvread will return massaged channels, where channel of the massaged channels is formed by averaging channels of the original data, starting at channel . ... If is specified as 0, then uvread will return as many channels as possible. object='reference' . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/miriad/progguide/node26.html -- 12.9 Кб -- 05.02.2013
Похожие документы

3. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/arlines.bluenearw
Mean dispersion = 1.10 angstroms / channel Start wavelength = 3412.81 angstroms End wavelength = 5389.50 angstroms Central wavelength = 4396.20 angstroms 42 lines identified from /data/maestro/bessell/sp505b Channel Wavelength Calculated Discrepancy Line # 73.7456 3491.3999 3491.4661 0.0662 1 100.5713 3520.4717 3520.5303 0.0586 2 123.7153 3545.5950 3545.6301 0.0352 3 189.9042 3617 ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/arlines.bluenearw -- 4.1 Кб -- 14.06.2001
Похожие документы

4. Old Calibration Data
... Wavelength Calibration . ... 30s wavecal plot . 30s flatfield plot . ... HeNeAr 4400 . B rQrtz 4400 . ... HeNeAr 4500 . ... BrQrtz 4200 . BrQrtz 4500 . ... These figures in the above table show the number of counts received from each of the lamps in a 30 second exposure with the 1.5 arcsec slit. ... Users have the option of taking calibration lamp data at the rotator angle of each object, but in many cases, it should be possible to measure the shift using observations of night sky lines. ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/arc35m/Instruments/DIS/old_cals.html -- 16.1 Кб -- 10.02.2012
Похожие документы
Еще в разделе: (Показать все результаты (>215) - www.apo.nmsu.edu/ )

5. IBIS - Description
... IBIS Instrumental Characteristics . ... Usable Wavelength Range . ... 2.5 frames/second @ 1024 x 1024(full-resolution) . 4 frames/second @ 512 x 512 (2 x 2 binning) . 4 frames/second @ 1024 x 512 (full-resolution) . ... Maximum Radial Wavelength Shift . ... Wavelength Drift of Transmission Profile . ... Wavelength Tuning Time . ... IBIS Fabry-Perot Characteristics . Fabry-Perot #1 . ... Nominal . ... Measured . ... 0.002 . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/solare/IBIS/ibis.description.html -- 8.4 Кб -- 03.04.2008
Похожие документы
Еще в разделе: (Показать все результаты (>8292) - www.arcetri.astro.it/ )

6. Channels (ImageJ API)
... Class . ... SUMMARY: NESTED | ... METHOD . ... public class Channels . ... Displays the ImageJ Channels window. ... Nested classes/interfaces inherited from class java.awt.Frame . ... Nested classes/interfaces inherited from class java.awt.Window . ... Nested classes/interfaces inherited from class java.awt.Container . ... Nested classes/interfaces inherited from class java.awt.Component . ... void . ... Methods inherited from class ij.plugin.frame. ... Methods inherited from class java.awt.Frame . ...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/plugin/frame/Channels.html -- 27.6 Кб -- 02.12.2010
Похожие документы

7. OYSTER Lab
The dimension (or index) of the data hyper-cube which is not to be used as loop-index when plotting all the selected data. Usually corresponds to X-axis selection, i.e. it is "pt" for "Time", or "ch" for channel/wavelength, etc. If plotting visibilities vs channel index, for example, selecting "ch" as slice would produce one plot per scan, unless the "All in 1" option is selected.
[ Сохраненная копия ]  Ссылки http://www.eso.org/~chummel/oyster/lab/amplitudes.m1.3.html -- 1.5 Кб -- 26.11.2007
Похожие документы
Еще в разделе: (Показать все результаты (>4786) - www.eso.org/ )

8. Limiting Energy Channels Input to the Fit
. Next: Multiple Data Sets Up: *fit* - Fit Data Previous: Two-Temperature Raymond Model . The energy range covered by the default channels depends on the instrument gain. To limit the fit to channels 7 to 30, specify the file with observed spectrum as: rp90[7:30] # will fit as before but using PSPC channels 7 to 30 # in the 34 binning scheme . rsdc@cfa.harvard.edu . 1998-06-10
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node150.html -- 3.5 Кб -- 01.10.2012
Похожие документы

9. SPUTNIK home page
... Resolution - 1.5-2.0 km . Swath - 450 km . ... Swath - 550 km . ... Resolution - 370 km . ... Spectral bands - 0.6-0.7 um; 0.8-1.1 um . ... Kondor - system for collection and transmission of data from sea and ice stations . ... Downlinking to ground stations (main centers) . ... Satellite's information system operates in both direct transmission mode and recording to on-board recorder mode with later downlink to ground station. ... For more information send a mail to: info@sputnik.infospace.ru . ...
[ Сохраненная копия ]  Ссылки http://sputnik.infospace.ru/ocean/engl/ocean_1.htm -- 8.3 Кб -- 27.12.2002
Похожие документы
Еще в разделе: (Показать все результаты (>11) - sputnik.infospace.ru/ )

10. Discovery Channel спонсирует постройку большого телескопа своего имени
... Сегодня: 10 апреля 2016 г. Компания Discovery Communications, которой принадлежит известный телевизионный канал познавательных программ Discovery Channel, стала спонсором разработки и строительства нового телескопа обсерватории Lowell в штате Аризона. ... Как было объявлено, основная миссия телескопа - это исследовательская работа и участие в научных программах NASA, Национального научного фонда и других подобных организаций. ... Шаттл Discovery стартовал . ...
[ Сохраненная копия ]  Ссылки http://news.cosmoport.com/2005/07/26/3.htm -- 22.7 Кб -- 10.04.2016
Похожие документы

11. Transmission of Sequences of Chaotic Samples Through RF Channel - Radiotekhnika
Radiotekhnika i elektronika, 1998, vol. ... Transmission of Chaotic Sample Sequences Through RF Channel . ... Received January 29, 1998 . ... The following set of operations is proposed for this purpose: transformation of the chaotic sample sequence into a sequence of AM pulses, modulation of high-frequency carrier by this signal, filtering out the high-frequency signal, demodulating it into a sequence of pulses, and retrieving estimates of the sequence of the chaotic samples. ...
[ Сохраненная копия ]  Ссылки http://www.cplire.ru/html/InformChaosLab/papers/trans.html -- 2.7 Кб -- 26.03.1999
Похожие документы

12. Fabry-Perot Interferometer: Data cubes
Fabry-Perot data cubes. Introduction: what is "data cubes"? Observations with the IFP consist of successive acquisition of a few dozen images of interference rings from the object (or from a calibration lamp) when changing the optical path between the flat-parallel plates. The radius of the rings is a function of wavelength and gap between the plates of the interferometer. ... Its interference rings of Ne line which use for phase calibration (convert object data to wavelength-scale). ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/lsfvo/devices/scorpio/ifp/cubes.html -- 7.1 Кб -- 26.05.2008
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/lsfvo/devices/scorpio/ifp/cubes.html -- 7.1 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/lsfvo/devices/scorpio/ifp/cubes.html -- 7.1 Кб -- 02.10.2012
Похожие документы

13. A Spectroscopy Exposure Time Calculator for IRAF
... Up: Iraf Packages . ... IRAF Group, NOAO 1 , PO Box 26732, Tucson, AZ 85726 . This paper describes a new IRAF spectroscopy exposure time calculator. ... SPTIME takes an input source spectrum, either a reference blackbody, power law, or a user spectrum, a background ``sky'', observing parameters such as exposure time, central wavelength, seeing, airmass, and moon phase, instrument parameters such as aperture sizes and detector binning, a description of the spectrograph, and desired output. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass99/P1-45/ -- 10.7 Кб -- 12.10.2000
Похожие документы

14. Image: Water is of great value on Tenerife. You can see irrigation channel
. Album : Фотоальбом Сергея Аюкова :: Travels to distant places and countries :: 1994/12 Tenerife, Canary Islands :: Walking to nearby mountain. It's only 1 km high but right from the sea level! . Up . << Prev . Water is of great value on Tenerife. You can see irrigation channel running around the mountain . Next >> . Created with the tool album from Marginal Hacks by David Madison on Wed Jun 5 20:38:28 2013 .
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/album/trips/1994.12.Tenerife/mountain/tn/hill07.jpg.index.html -- 5.4 Кб -- 05.06.2013
Похожие документы
Еще в разделе: (Показать все результаты (>202) - crydee.sai.msu.ru/ )

15. Optical static Fourier spectrometer
Static Fourier spectrometers are often used for spectral measurements of the ionosphere emissions. There are two main advantages of Fourier spectrometers (FS) - large geometric factor and high spectral resolution; these parameters are two orders better than for grating spectral instruments. ... In scanning Fourier spectrometer optical and electric modulation of signal is used to avoid this problem, for static Fourier spectrometer there are no such ways. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/~lapchuk/my_web/Spectrometer.htm -- 10.1 Кб -- 21.02.2000
Похожие документы

16. Hunt For Aliens On National Geographic Channel - an Astronomy Net UFO Forum
UFO Forum Message . Forums: . ... God and Science ћ SETI ћ Software ћ UFO ћ XEphem . ... Discussion Forums | ... Hunt For Aliens On National Geographic Channel . Forum List | ... Hunt for Aliens premieres Thursday, April 1st at 8 PM ET on the National Geographic Channel. ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/forums/ufo/messages/1099.shtml -- 14.0 Кб -- 09.04.2016
Похожие документы

17. http://www.mrao.cam.ac.uk/~dag/UVFLP/ReadMe.txt
Note: a new task -- "FLOPM" -- is available in recent versions of AIPS (31DEC07 and later), which also reverses the order of spectral channels, making UVFLP as described below unnecessary. ... UVFLP (to re-order channels in GMRT LSB uv data files within AIPS) ================================================================== To flip the oder of spectral channels in uv databases in AIPS. ... 1) Original data: 128 <--- channels <--- 1|1 ---> channels ---> 128 ------------------------|- LSB | ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~dag/UVFLP/ReadMe.txt -- 5.9 Кб -- 08.06.2012
Похожие документы

18. http://www.iki.rssi.ru/seminar/20100225/evdokimova.pdf
... indices rather than retrieve abundances: 1.2, 1.5, 2.0 µm · Work with calibrated radiances rather than relative spectra · Ad hoc atmospheric corrections Spectral index : S( ABCD) - S1 Index = S( ABCD) Correction on atmospheric absorption ·MOLA topography ·CO2: p,T ­ from European Mars Climate Database ·H2O column (Ls, ) - from TES observations ·H2O (, l, z) ­ from GFDL MGCM model ·HITRAN(2004) OMEGA DETECTOR C Wavelength,µm Errors and uncertainities ...
[ Текст ]  Ссылки http://www.iki.rssi.ru/seminar/20100225/evdokimova.pdf -- 1566.0 Кб -- 23.03.2010
[ Текст ]  Ссылки http://www.cosmos.ru/seminar/20100225/evdokimova.pdf -- 1566.0 Кб -- 23.03.2010
Похожие документы

19. SMIS IKI RAN (Sample Images / Miscellaneous)
... SMIS ] . ... Aqua, 22.04.2004, 04:15 GMT . ... Space Research Institute, Moscow ( http://smis.iki.rssi.ru/ ) . NOAA 12, 3.04.2004, 13:20 GMT . ... NOAA 16 20/08/2003 3:09 GMT . ... NOAA 16 4/04/03 10:41 GMT . ... NOAA 15 1999.12.14 09:32 MSK . ... NOAA 15 . ... NOAA 14 22/01/1999 9:13 GMT . ... Pseudo-colour image. ... Red - channel 5, Green - channel 2, Blue -channel 1 . ... True-color composition from NOAA 12 and NOAA 14 AVHRR Channel 3 data using images acquired at different times of a day. ...
[ Сохраненная копия ]  Ссылки http://smis.iki.rssi.ru/images/mix/m_samp_e.htm -- 19.6 Кб -- 12.02.2005
Похожие документы

20. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... We have obtained imaging polarimetry of the comet C/2013 R1 (Lovejoy) with 2-Channel-Focal-Reducer Rozhen instrument at 2m RitcheyтАУChr tienтАУCoud telescope of the Bulgarian National Astronomical Observatory Rozhen in two dust continuum filters covering wavelength intervals clear from molecular emissions and centred at 4430 in blue filter and at 6840 in red filter. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/highlights/2015/675.html -- 5.5 Кб -- 03.08.2015
Похожие документы
Еще в разделе: (Показать все результаты (>580) - star.arm.ac.uk/ )

1 | 2 | 3 | 4 | 5 | След.


Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам

Комментарии, вопросы? Пишите: info@astronet.ru или сюда

Rambler's Top100 RFBR Яндекс цитирования