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1. SAO RAS home page
... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...
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Ссылки http://www.sao.ru/ -- 11.4 Кб -- 09.04.2016
[ Сохраненная копия ] Ссылки http://mavr.sao.ru/ -- 11.4 Кб -- 09.04.2016
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2. High Spatial Resolution Mid- and Far-infrared Imaging Study of NGC 2346
We present the first high spatial resolution mid-IR and far-IR images of the planetary nebula NGC 2346 using the Multiband Imaging Photometer for Spitzer (MIPS) on board the Spitzer Space Telescope. The morphology at 24 ЮМm is strikingly similar to that seen in the optical image, with an additional unresolved hot dust component at the center. ... ADS Citation Query . citations = 31 . citations vs. year [year,citations] . ...
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Ссылки http://www.stsci.edu/~kgordon/papers/2004ApJS..154..302S.html -- 4.2 Кб -- 21.01.2016
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3. HIGH RESOLUTION IONOSPHERIC MASS SPECTROMETER P-11
HIGH RESOLUTION IONOSPHERIC MASS SPECTROMETER P-11 . ... Onboard mass-spectrometric equipment for study of neutral and ionized components of Earth upper atmosphere. Mass-spectrometer P-11 is one of P-series modifications of the on board radio-frequency monopole spectrometers. ... The instruments of P-series have passed successful approbation in space experiments aboard geophysical rockets MP-12, launched for investigation of Earth upper atmosphere (Ref. ... Measured mass number range, AMU - 1.. ...
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Ссылки http://space.univ.kiev.ua/projects/warning/p-11.html -- 5.7 Кб -- 15.02.2000
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4. NICMOS and the VLT: A New Era of High Resolution Near Infrared Imaging and
... ST-ECF, ESO, STScI and the NICMOS IDT organized a workshop on near infrared imaging from space and ground was held in Pula on May 26-27, 1998. ... The meeting was held in May 1998, about one year after science observations started with NICMOS, and about half a year before the Infrared Spectrometer and Array Camera (ISAAC) starts to operate on the VLT. Currently, it is expected that NICMOS will operate until the end of 1998. ...
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Ссылки http://www.stecf.org/conferences/meeting/ -- 4.8 Кб -- 13.06.2006
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5. http://www.mrao.cam.ac.uk/~anthony/latex/Ogawa.ps
The Initial Condition of Cosmological High-Resolution Simulations T. Ogawa et al. ... However, the resolution of their INITIAL conditions is not high. ... The reso- lution of these initial conditions are constrained by the mesh size, in other words, high-frequency components of (x) are neglected initially. We argue the need for cosmological high-resolution sim- ulations to use a high-resolution initial condition, in other words, an initial condition including high-frequency components. ...
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Ссылки http://www.mrao.cam.ac.uk/~anthony/latex/Ogawa.ps -- 20.0 Кб -- 24.06.2000
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6. AO on AR 8970
On April 27 the large sunspot in Active Region 8970 was observed using the Adaptive Optics system at the Swedish Vacuum Solar Telescope at La Palma. ... It showed to give a significant improvement of the image quality under less favorable conditions. Click on the image to get a high resolution version. ... The data cube is cut in three pieces to get manageable file sizes, you can glue them together to restore the whole 108 images cube. gband_ao.01_36.cube.fits 36.5 Mb: image 1 - 36 . ...
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Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/sun/lightbridges_svst_big.htm -- 5.4 Кб -- 22.12.2000
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7. Chief Designers Council for Russian piloted programs Resolution No. 285-01/06...
... After hearing and discussing Rocket-Space Corporation Energy General Designer U.P.Semevov's report on the fulfilling the flight program of the orbital complex Mir and proposals on its further exploitation, the Council draws attention to: . ... According to the Russian Government Resolution No. 76 of January 21, 1999 a large amount of work to find and attract Russian and foreign investments to provide the further exploitation of the orbital station Mir was carried out. ...
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Ссылки http://www.cosmoworld.ru/mirstation/english/documents/constructors_010699.shtml -- 9.7 Кб -- 09.04.2016
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8. Optimization of spectroscopic observations
... Let us first find out which way -- rise in spectral resolution with some loss in the S/N ratio or increase in the S/N ratio with a fixed spectral resolution -- is better for the purpose of reduction of equivalent width determination errors. ... N -- number of counts for 1 ? ... line equivalent width, . ... Thus if the spectral resolution is managed to be increased (i.e. to decrease )without loss in the number of counts falling at 1 ?, the equivalent width measurement error is then proportional to . ...
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Ссылки http://mavr.sao.ru/hq/ssl/PFES/node2.html -- 13.9 Кб -- 02.10.2012
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9. Infrared and Sub-millimetre Observing Conditions on the Antarctic Plateau
... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Parkes radio telescope . ... Information & tools for observers . ... Infrared and Sub-millimetre Observing Conditions on the Antarctic Plateau . ... The Antarctic plateau provides the best terrestrial sites for infrared and sub-millimetre astronomy. ... Finding a location where aerosol levels are minimised is a key constraint in determining the optimum site on the Antarctic plateau for an infrared observatory. ...
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Ссылки http://www.atnf.csiro.au/pasa/17_3/hidas/paper/index.html -- 51.7 Кб -- 08.04.2016
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10. http://www.sao.ru/drabek/CCDP/TAPER/HTM_resume/PixVision/specim.pdf
... Imaging Spectrograph For Visible And Near Infrared (NIR) Spectral Ranges n High-Efficiency Holographic Grating n First Direct-Sight C-Mount Imaging Spectrograph n Polarization Independent n Specim Ltd. ImSpectorTM Ima ging Spectr o g raph General Description The ImSpector adds spectral resolution to conventional imaging cameras via a standard Cmount. ... The ImSpector N17, Specim's latest imaging spectrograph, is designed for NIR imaging in 900 - 1750 nm with InGaAs matrix cameras. ...
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Ссылки http://www.sao.ru/drabek/CCDP/TAPER/HTM_resume/PixVision/specim.pdf -- 81.6 Кб -- 25.09.1998
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11. NVFlex
... NVFLEX . ... NIGHT VISION DEVICES . ... CAMERAS . ... Home Products Night Vision Devices NVFlex . The NVFlex™ is LOMO’s latest Night Vision Device . It can be used either as a handheld monocular or attached to a 35mm/digital camera or camcorder attachment . ... The kit includes the projection eyepiece, and camera/camcorder adapter rings (37mm, 40.5mm, 46mm, 49mm, 52mm) . ... Camera/Camcorder Adapter Rings . Other adapter rings are available from your local camera/camcorder retailer . ...
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12. High Resolution HST Images of Pluto and Charon (ESO Press Release 09/94)
... The remote planet Pluto and its moon Charon orbit the Sun at a mean distance of almost 6,000 million kilometres, or nearly fourty times farther out than the Earth. During a recent investigation by an international group of astronomers [1], the best picture ever of Pluto and Charon [2] was secured with the European Space Agency's Faint Object Camera at the Hubble Space Telescope (HST). ... The new HST image was taken when Charon was near its maximum elongation from Pluto (0.9 arcseconds). ...
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Ссылки http://www.eso.org/~ohainaut/nice/pluto.html -- 8.5 Кб -- 18.08.2004
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13. Кудашев Ефим
Кудашев Ефим .Б орисович ., ... 2009. ... Шум турбулентных потоков определяется структурой турбулентных пульсаций давления. ... В представленных работах выполнено исследование распределения энергии турбулентных пульсаций одновременно и по временным частотам, и по волновым числам (пространственным масштабам) поля турбулентных давлений. ... Методы волновой фильтрации применены для исследования регистрации мелкомасштабных компонент турбулентных пульсаций при воздействии вибраций и акустических шумов. ...
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Ссылки http://www.iki.rssi.ru/comp/2009/Kudashev.htm -- 23.9 Кб -- 30.10.2009
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/comp/2009/Kudashev.htm -- 23.9 Кб -- 30.10.2009
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14. Towards a General Definition for Spectroscopic Resolution
... Judged by their instrumental profiles, spectrometers fall into two basic classes---Lorentzian and Gaussian---with many other line profile functions (sinc functions, Voigt functions, Airy functions, etc.) falling into one of these two categories in some limit. We demonstrate that the Rayleigh, Sparrow, and Houston resolution criteria are of limited use compared to the ``equivalent width'' of the line profile. ... Rayleigh criterion. ... All of these functions have continuous higher derivatives. ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/jonesa.html -- 12.2 Кб -- 03.11.2000
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15. Energy resolution
Next: Detection Efficiency Up: CCD Scientific Performance Previous: CCD Scientific Performance . The X-ray energy required to liberate a charge pair in a semiconductor is approximately an order of magnitude lower than in gas detectors, hence the potential spectroscopic advantage of CCD detectors. ... For a number of years, good scientific CCDs attained noise performance of electrons rms, but this limited the energy resolution for X-ray energies 3keV. ...
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Ссылки http://xmm.vilspa.esa.es/user/socpub/ccd_review/node5.html -- 12.5 Кб -- 30.08.1996
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16. Gemini Near-Infrared Integral-Field Spectrograph (NIFS) Spectrograph.
... Thus all regions of the 0.94-2.50 micron wavelength range accessible from Mauna Kea can be recorded using five fixed angle gratings. ... Grating Angle . ... Efficiencies for the NIFS gratings are shown above. The NIFS spectrograph uses a Bouwers collimator and a refractive camera. ... With these assumptions, the NIFS system efficiency including the Gemini telescope optics but excluding the transmission of the adaptive optics system is about 0.17 e - /photon at J , and 0.22 e - /photon at H and K . ...
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Ссылки http://www.mso.anu.edu.au/nifs/description/spectrograph.shtml -- 7.9 Кб -- 02.10.2012
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17. XWare > APOD
... Space Weather forcasters are predicting major storm conditions over the next few days as the active Sun has produced at least three strong flares and a large coronal mass ejection (CME) since Tuesday, June 6th. Up Close to Jupiter's Moon Io . ... Above is the highest resolution photograph yet taken of the Solar System's strangest moon. The surface of Jupiter's moon Io is home to violent volcanoes that are so active they turn the entire moon inside out. ... The Very Large Array Turns Twenty . ...
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Ссылки http://www.astronet.ru/db/xware/apod.html?page=64&d=2002-02 -- 15.1 Кб -- 12.04.2016
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18. Resolution - an Astronomy Net ATM Forum Message
ATM Forum Message . Forums: . ... Post . ... Resolution . Forum List | ... Post Message | ... Posted by Rick Crockett on April 25, 2007 08:46:54 UTC . ... resolution - aschilli - April 30, 2007 - 00:08 UTC . Indoor resolution - rick_crockett - June 2, 2007 - 07:04 UTC . ... 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" . ...
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19. International Astronomy Olympiad 2010, resolutions
... Resolution to be issued: . For reports, received before June 11: not later than 15 days after receiving . For reports, received on June 12-21: not later June 27 . For reports, received on June 22 - June 27: not later July 27 . For reports, received on June 28 - July 16: during the week July 26-30 . For reports, received on July 17-31: not later 4 weeks after receiving . ... Dr. Michael G. Gavrilov, Founding Chairman and Coordinator of the International Astronomy Olympiad (IAO) . ...
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Ссылки http://www.issp.ac.ru/iao/2010/ia10rt_e.html -- 9.6 Кб -- 30.08.2010
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20. ARC 3.5m | Instrumentation
... ARC 3.5m | Instrument Summary . ... ARCES (Echelle) : the ARC Echelle spectrograph, a high resolution (R~31,500) echelle spectrograph that observes the entire wavelength range from 3200 е to 10000 in a single image on a 2048x2048 CCD. This instrument is permanently mounted at the NA1 port. ... In addition to the facility instruments, several visitor instruments have been used at the 3.5m, and some of these are available to the ARC observing community by contacting the instrument PIs: . ...
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Ссылки http://www.apo.nmsu.edu/arc35m/Instruments/Instrumentation_ARC35m.html -- 7.5 Кб -- 09.10.2014
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