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61. Trajectory report
... The OC "Mir" orbit parametres before the final burns . ... Orbit period (in min) . ... Mean orbit altitude (km) . ... solar F 10.7 flux . ... F 10.7 <= 100 - low level; 100 < F 10.7 < 150 - medium level; F 10.7 >= 150 - high level . Orbit 86328(15) - the first burn bulding the descent orbit  D V 1 =9.3 m/s. After burn altitude H min = 188.2 km, H max = 219.2 km. Orbit 86329(16) - the descent orbit second impulse D V 2 =10.4 m/s. After burn altitude H min = 158.9 km, H max = 218.5 km. ...
[ Сохраненная копия ]  Ссылки http://www.mcc.rsa.ru/www_old/Mir/www_eng/MIR/BNO/spr.htm -- 17.2 Кб -- 28.05.2014
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62. http://www.winer.org/Downloads/astro-ph-KELT-3b.pdf
... Table 1 lists all RV data for KELT-3 , and Figure 2 shows 20 TA B L E 1 RV O B S E RVAT I O N S O F K E LT- 3 BJD RV RV errora Source (TDB) (m s-1 ) (m s-1 ) 2455983.672916 -319 25 TRES 2455990.777987 -66 14 TRES 2456000.473809 -31 27 FIES 2456001.465355 103 20 FIES 2456002.514673 -259 20 FIES 2456003.552533 90 16 FIES 2456004.432251 0 16 FIES 2456018.656206 -324 14 TRES 2456019.709404 4 19 TRES 2456020.710562b -125 18 ... Both observations were able to resolve KELT-3 from...
[ Текст ]  Ссылки http://www.winer.org/Downloads/astro-ph-KELT-3b.pdf -- 1862.3 Кб -- 06.12.2013
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63. 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. ...
[ Сохраненная копия ]  Ссылки http://www.vista.ac.uk/observing/etc/index.html -- 15.1 Кб -- 28.03.2013
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64. Star Formation History
... A model for the chemical evolution of a disk galaxy is presented. The model reproduces all the basic . ... investigations of the star formation history. ... the galaxyЫand incorporating a delay in the onset of star formation make it possible to model different scenar- . ios for the evolution of a galaxy's luminosity. ... evolution of massive galaxies. ... of reconstructing the star-formation history and galactic luminosity from observations of galaxies at different . ...
[ Сохраненная копия ]  Ссылки http://www.inasan.rssi.ru/~dwiebe/abstracts/sfrazh.html -- 2.9 Кб -- 27.09.2012
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65. http://www.gpad.ac.ru/collaborations/inasan.pdf
The new view on the population of Galactic open clusters A.E.Piskunov1, N.V.Kharchenko2, S.RЖser3, E.Schilbach3, R.-D.Scholz4 1 2 3 4 Institute of Astronomy, Moscow, Russia Main Astronomical ... Observatory, Kiev, Ukraine Astronomisches Rechen-Institut, Heidelberg, Germany Astrophysikalisches Institut Potsdam, Germany What are open clusters and what do they teach us Groups of Population I ... Cluster complexes: OCC-1 = Gould's Belt cluster complex? ...
[ Текст ]  Ссылки http://www.gpad.ac.ru/collaborations/inasan.pdf -- 2655.7 Кб -- 05.07.2006
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66. Phil Plait's Bad Astronomy: Mad Science
... Bad Astronomy . ... Mad Science . ... Universe Today . ... Keep Bad Astronomy close to your heart, and help make me filthy rich. ... type 1a supernovae seem most useful . ... This is a bright, massive star that explodes after fusing all the light elements in its core. ... That means we can calculate how far away it is. ... This is exactly what we are trying to do with these supernovae; look far enough away that any deviations from flatness of the Universe can be seen. ... Phil Plait . ...
[ Сохраненная копия ]  Ссылки http://www.badastronomy.com/mad/1998/omega0_sn.html -- 20.5 Кб -- 09.04.2016
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67. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB3F66957-8E2C-433C-BFCA-E35D3587A356%7D
. The picture illustrates the new capabilities of Apertif. The circles show the location on the sky of the two pulsars detected simultaneously, separated from each other by about seven times the diameter of the full Moon. The Moon indicates the field of view of the old WSRT: it can detect sources only if they are closer to each other than a distance similar to the apparent size of the full Moon. The inset on the left shows the average time profile of the pulsars detected. Illustration: ASTRON
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB3F66957-8E2C-433C-BFCA-E35D3587A356%7D -- 3.8 Кб -- 10.04.2016
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68. http://master.sai.msu.ru/media/presentations/2012/arXiv05oct12_1.doc
... Using the CFBDSIR wide field survey for brown dwarfs, we identified CFBDSIRJ214947.2-040308.9, a late T dwarf with atypically red J-Ks colour. ... SN 2009ip in NGC 7259 Electronic Telegram No. ... 7.09, [19.0; 2009 Aug. ... Accepted for publication in MNRAS Subjects: High Energy Astrophysical Phenomena (astro-ph.HE) The jet opening angle theta_jet and the bulk Lorentz factor Gamma_0 are crucial parameters for the computation of the energetics of Gamma Ray Bursts (GRBs). ...
[ Текст ]  Ссылки http://master.sai.msu.ru/media/presentations/2012/arXiv05oct12_1.doc -- 81.0 Кб -- 07.10.2012
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69. Malinovsky Alexandre Mikhailovich, Astro Space Center (ASC)
... Department Number . ... Astro Space Center . ... Telephone Number . 7(495) 333 3366 . FAX Number . 7(495) 333 2378 . ... amalin@lukash.asc.rssi.ru . ...
[ Сохраненная копия ]  Ссылки http://lukash.asc.rssi.ru/people/amalin.htm -- 3.3 Кб -- 06.10.2010
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70. Heracles
... Heracles Triplane and Aerospace Systems . The key characteristics of two-stage aerospace systems are determined according to speed and carrying capacity of the aircraft-carrier used . ... So the SPIRAL system hypersonic carrier was expected to launch the second stage by weight 63 tons at a speed corresponding to 6M; whereas launching weight of the MAKS system orbital stage with the use of the An-225 MRIYA heavy subsonic aircraft reaches 275 tons, and the HERACLES aircraft - 450 tons. ...
[ Сохраненная копия ]  Ссылки http://www.buran.ru/htm/heracles.htm -- 10.6 Кб -- 01.10.2012
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71. Images of Supernova 1998bu in M96
Images of Supernova 1998bu in M96 . ... It took less than 24 hours for me to accumulate enough images of SN 1998bu in M96 to run out of space on the main page. ... Optical Light Curve of the Type Ia Supernova 1998bu in M96 and the Supernova Calibration of the Hubble Constant by Nicholas B. Suntzeff et.el. SAOTNG images . ... AUDE SN 1998bu light curves in French [ Translate ] . ... The light curve is an assemblage of submissions of the event's rise and decay in the R, V, and Visual band. ...
[ Сохраненная копия ]  Ссылки http://www.rochesterastronomy.org/SNIMAGES/sn1998bu.html -- 30.1 Кб -- 10.04.2016
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72. http://site2010.sai.msu.ru/static/doc/GHerriot_site2010.ppt.pdf
Using Site testing data for Adaptive Optics simulations Kislovodsk, October 2010 1Glen Herriot, 1David Andersen, 1Jean-Pierre VИran, 2Brent Ellerbroek, 2Luc Gilles, 2Lianqi Wang 1National Research Council Canada ­ Herzberg Institute of Astrophysics 2TMT Project Office, Pasadena TMT.AOS.PRE.10.074.REL01 1 Outline TMT / NFIRAOS Site Testing Parameters and their value for Adaptive Optics Simulations ... TMT.AOS.PRE.10.074.REL01 9 What is the interest of Adaptive Optics in r 0 Seeing ? ...
[ Текст ]  Ссылки http://site2010.sai.msu.ru/static/doc/GHerriot_site2010.ppt.pdf -- 1942.1 Кб -- 18.10.2010
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73. XV-AVHRR
... Satellite data ] . SMIS ] . The program is designed to process the specific AVHRR instrument data for calculation and analysis of temperature fields on the sea surface and upper level of clouds. It performs brightness correction for visible channels with regards to clouds altitude. ... The program features a wide variety of classification algorithms (including two-dimensional histogram analysis) and enables to construct personal procedures for classification. ... Back to SMIS Home Page . ...
[ Сохраненная копия ]  Ссылки http://smis.iki.rssi.ru/inform/engl/soft/e_avhrr.htm -- 3.5 Кб -- 13.03.1997
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74. 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
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75. SETI Assumes ET Doesnot Care About Can Being Detected What If - an Astronomy
Astronomy Discussion Forums . ... God and Science ћ SETI ћ Software ћ UFO ћ XEphem . ... SETI Assumes ET Doesnot Care About Can Being Detected What If . ... Post Message | ... My search on how to go undetected in space and SETI Search for Extraterrestrial Intelligence SETI. ... 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/seti/messages/34.shtml -- 15.1 Кб -- 09.04.2016
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76. Astronaut Bio: Richard F. Gordon
... Richard F. Gordon, Jr. ... NASA Astronaut (former) . ... ORGANIZATIONS: Fellow, American Astronautical Society; Associate Fellow, Society of Experimental Test Pilots; and Navy League. ... Gordon, R. F., FJ-4B FUEL CONSUMPTION AND PERFORMANCE REPORT, Flight Test, NAS Patuxent River, Maryland, 1958. ... In 1957, he attended the Navy's Test Pilot School at Patuxent River, Maryland, and served as a flight test pilot until 1960. ... He served as backup pilot for the Gemini 8 flight. ...
[ Сохраненная копия ]  Ссылки http://www.jsc.nasa.gov/Bios/htmlbios/gordon-rf.html -- 11.0 Кб -- 07.07.2015
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77. Symbolic circuit processor
... All circuit parameters have been presented in a symbolic form. ... To use the program you will need a CIR file (PSpise, DesignLab file) of your circuit. CIR file examples have been enclosured: bpasside.cir, test1.cir, test2.cir, test3.cir, test4.cir, laksamp.cir, bridge.cir, uA741acf.cir, quartz.cir. ... Ideal operational amplifier (nullor) * Nname n1 n2 n3 n4 * * In the ideal op amp data, (n1,n2) represent output nodes, * (n3,n4) represent input nodes (noninverting, inverting). ...
[ Сохраненная копия ]  Ссылки http://astrometric.sai.msu.ru/~symbol/cirsym.html -- 4.4 Кб -- 06.10.2004
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78. Scientific.ru Альтернативный форум
Альтернативный форум . Scientific.ru Все форумы . ... valia - 23.01.2007 15:59 . ... вернуться на форум ] . ... Задача о движении трех тел... valia, 22.01.2007 10:52 . Re: Задача о движении трех тел решена Зундманом в 1908-13 Уникум, 22.01.2007 13:54 . ... Re: По рабоче-крестьянски, для любых трех тел... valia, 22.01.2007 17:01 . ... Re: Задача о движении трех тел... drevnij, 22.01.2007 11:31 . ... Философ - это тот, для кого задача трех тел неразрешима :) (-) Hyperboloid, 22.01.2007 15:31 . ...
[ Сохраненная копия ]  Ссылки http://www.scientific.ru/dforum/altern/1169557182 -- 18.7 Кб -- 12.04.2016
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79. http://vast.sai.msu.ru/lk/
Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Phase range for plots: -0.5 to 1.0 0.0 to 2.0 0.0 to 1.0 . ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... Two period search methods are currently implemented. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . ...
[ Сохраненная копия ]  Ссылки http://vast.sai.msu.ru/lk/ -- 6.4 Кб -- 18.08.2015
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80. 2dF QSO Redshift Survey (2QZ)
The 2dF QSO Redshift Survey (2QZ) . ... Before jumping into all the finer details of teh survey, a brief non-astronomer's guide to redshift surveys is available. ... The primary scientific aims of the QSO survey are: (1) to obtain the primordial fluctuation power spectrum out to COBE scales, (2) to determine the rate of QSO clustering evolution in the non-linear and linear regimes and hence obtain new limits on the value of and the bias parameter, (3) to apply a powerful geometric method to measure . ...
[ Сохраненная копия ]  Ссылки http://www.2dfquasar.org/ -- 7.8 Кб -- 17.06.2008
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