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61. 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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62. 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 ? ...
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Ссылки http://site2010.sai.msu.ru/static/doc/GHerriot_site2010.ppt.pdf -- 1942.1 Кб -- 18.10.2010
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63. http://www.uafo.ru/publ/gao/2012GAOconf_289_292_Mozharovsky.pdf
sw@newmail.ru THE PROBE LAYER METHOD IN THE CALCULATIONS OF CONTRIBUTION AND RESPONSE FUNCTIONS S.G.Mozharovsky Ussuriysk Astrophysical Observatory of FEB RAS, Ussuriysk, Russia sw@newmail.ru The method of probe layer for the calculation of response and contribution functions is discussed. ... This allows us to turn from the response functions to the contribution functions calculated with help of the probe layer (CFPL). ... V- VMAX . ... Solar Phys., v.136, p.239-250. ... Solar Phys., v.35, p.11-29. ...
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Ссылки http://www.uafo.ru/publ/gao/2012GAOconf_289_292_Mozharovsky.pdf -- 269.8 Кб -- 15.01.2013
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64. Астронет > Archive of Astronomical and Astrophysical Transactions
... Астронет | ... The formation of chemical peculiarities in stellar atmospheres . ... Asymmetry in the variability of radio sources towards the centre and anti-centre of the galaxy . ... Mathematical methods in studying the structure and dynamics of gravitating systems . ... Mathematical methods in studying the structure and dynamics of gravitating systems: Preface . ... On the astronomical applications of the dynamics of hierarchical systems . ... Dynamics of gaseous disks of spiral galaxies . ...
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Ссылки http://www.astronet.ru/db/AATr/cont07.html -- 20.7 Кб -- 28.02.2014
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65. New technique measures mass of exoplanets | Astronomy.com
... New technique measures mass of exoplanets . ... Now, scientists at the Massachusetts Institute of Technology (MIT) have developed a new technique for determining the mass of exoplanets using only their transmission spectra dips in light as a planet passes in front of its star. ... To determine the mass of an exoplanet using transmission spectroscopy, de Wit relied on the effect that a planet s mass has on its atmosphere, as transmission spectra give information on a planet s atmospheric properties. ...
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Ссылки http://www.astronomy.com/news/2013/12/new-technique-measures-mass-of-exoplanets -- 71.7 Кб -- 10.04.2016
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66. MASTER-II Kislovodsk
M obile A stronomical Sy stem of TE lescope- R obots MASTER-II Kislovodsk Lomonosov Moscow State University, Sternberg Astronomical Institute , Moscow Union "Optic" , Kislovodsk Solar Station Latitude = 43 o љ44'.767љN; Longitude = 42 o љ31'.417љE; Altitude = 2067љm MASTERљIIљ(8љsquareљdegress) + MASTERљVWF(VeryљWideљFieldљCameras (FOV=800 square degrees, Timeљresolutionљupљtoљ150љms, with unfiltered m_lim=14m on 5 sec. exposure, and ~10.5m with 0.15 sec) . ... 11h 38m 38.0s , -09d 59m 59s) . ...
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67. http://vega.inp.nsk.su/~inest/workbbeam/cbb.ps
SLIDE 1 Coherent beambeam e#ects study. ... He has shown that a finite length (in other words equal to # # ) of colliding bunches can lead to the coupling of synchrobetatron modes in the beambeam system, and thus a headtail type instability of colliding bunches may arise. ... These modes have been observed in di#erent machines. ... SLIDE 5 Figure shows the dependence of the measured and calculated synchrobetatron mode tunes on the beam current for equal electron and positron bunch intensities. ...
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Ссылки http://vega.inp.nsk.su/~inest/workbbeam/cbb.ps -- 70.9 Кб -- 18.06.2001
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68. The Pul-3 astrometric catalogue (Second edition). Data access form.
The starting page - The catalogues page - The list of the PUL2 fields - The list of the Pul-3(Pul-3SE) fields - The list of the PUL_ERS fields . please read short description of the access form controls . ... Right Ascension (ICRF/Tycho-2) J2000 at the central epoch of obs. (hours, minutes, seconds) (Obligatory parameter) . ... proper motion in RA (*cos(DE)) (ICRF/Tycho-2). (mas/yr) . ... Check the apropriate checkbox to output these data and radiobutton to select stars within interval. ...
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Ссылки http://www.puldb.ru/pul3/pul3f.php?fn=001&ra=00%2009%2008.6&de=+27%2045%2047 -- 15.1 Кб -- 09.04.2016
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69. ASP: An Ancient Universe - The Age of the Oldest Stars
An Ancient Universe: How Astronomers Know the Vast Scale of Cosmic Time . ... b) The Age of the Oldest Stars . The Sun The Sun and other stars shine by converting superheated hydrogen in their centers into helium in a process called thermonuclear fusion. ... In this way, we can measure the ages of certain stars. ... The Ancient Universe - The Age of the Expanding Universe - The Age of the Oldest Stars - The Age of Light From Distant Galaxies - The Age of the Chemical Elements | ...
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Ссылки http://www.astrosociety.org/edu/publications/tnl/56/ancient2.html -- 8.4 Кб -- 02.10.2012
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70. 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. ...
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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
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[ Сохраненная копия ] Ссылки http://saistud.sai.msu.ru/poisk/ -- 122.2 Кб -- 21.02.2016
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71. J2357-1125
... 5-GHz total flux density . ... 1.4 Jy . ... 0.960 * = the position has been determined to an accuracy of 10 mas from the VLBApls data . VLBApls image at 5 GHz . color gif | contour gif | ... Correlated flux density (Jy) vs. projected baseline length plot . gif | ... flux density (Jy) . EW position (mas) . ... major axis (mas) . minor axis (mas) . position angle ( ) . ... VLBApls reference: Fomalont et al. ... VLBApls home page . ...
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Ссылки http://www.vsop.isas.ac.jp/VLBApls/J2357-1125.htm -- 3.6 Кб -- 08.05.2001
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72. GLOOBUS-M diagnostics
The low aspect ratio, or spherical tokamak Globus-M [1] has recently been built in a support of international spherical tokamak plasma investigation program. ... The survey to determine the work scope in diagnostic design for Globus-M is given in the paper. ... The next one is an advanced diagnostic set intended to supply the data on basic plasma parameters: electron temperature and density profiles, ion temperature, plasma composition, radiation profile, Zeffective. ... Magnetic Diagnostics. ...
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Ссылки http://www.ioffe.rssi.ru/HTPPL/GLOBUS-M/diagnostics.html -- 20.0 Кб -- 17.10.2012
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73. The new concept of formation and development of the Solar system
... part 2 | ... Part 1 . The new concept of formation and development of the Solar system. ... Thus, the initial pulse of the rotation of a protosolar cloud of the solar system was determined as a result of the diversion of a part of the moment of the rotational pulse of the Galaxy. ... Besides this new approach to the pre-solar system as a system of the destroyed vortex structure, we can understand now a number of other peculiarities of the Solar system's structure. ...
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Ссылки http://www.lermus.ru/users/trunaev/part1.htm -- 28.0 Кб -- 04.12.2001
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74. Tatjana Khruzina
... For the past years I have been working on the problem of synthesis of light curves of close binary systems, consisting of a normal star and a compact object (point object with fixed X-ray luminosity). ... Possible existence of a bright spot on the disk's lateral surface is taken into account. ... The last of then will be published in Gordon and Breach Publishers ( Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ... Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ...
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Ссылки http://uranus.sai.msu.ru/~kts/ -- 4.4 Кб -- 22.09.2000
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75. Информация для прессы
... In accordance with the de-orbit plan the OC "Mir" is in a waiting mode continuing its deceleration in Earth atmosphere. During the previous day the OC "Mir" onboard systems were subject to a routine check out, the current trajectory parametres were registered. The processed information confirms the MCC readiness for the final stage dynamis operations with the OC "Mir". ... The first corrective impuls ( the cargo ship "Progress M1-5" 8 control engines are fired): . T burn start - 03.32; . ...
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Ссылки http://www.mcc.rsa.ru/www_old/Mir/www_eng/MIR/BNO/Arhiv/Inform_press2103.htm -- 14.9 Кб -- 28.05.2014
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76. Astronaut Bio: Mark C. Lee 10/2006
... Mark C. Lee (Colonel, USAF, Ret.) NASA Astronaut (former) . ... EDUCATION: Graduated from Viroqua High School, Viroqua, Wisconsin, in 1970; received a bachelor of science degree in civil engineering from the U.S. Air Force Academy in 1974, and a master of science degree in mechanical engineering from Massachusetts Institute of Technology in 1980. ... NASA EXPERIENCE: Lee was selected as an astronaut candidate by NASA in May 1984. ... Lee retired from NASA and the Air Force effective July 1, 2001. ...
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Ссылки http://www.jsc.nasa.gov/Bios/htmlbios/lee.html -- 9.3 Кб -- 07.07.2015
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77. Institute of Cosmical Research and Aeronomy
Main News Phones Research area Brief history Institute Structure Experimental Base Observational data English/Russian . research on the site(Google) . ... 7(4112)390400 . Fax: . 7(4112)390450 . ... Division of Aeronomy . ... Phone: +7(4112) 39-04-48 . Fax: +7(4112) 39-04-50 . ... solar-terrestrial physics . magnetosphere physics . ... Laboratories: . Geomagnetism Laboratory . Ionosphere Physics Laboratory . ... Ionosphere and Magnetosphere Radioemission Laboratory . ...
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Ссылки http://ikfia.ysn.ru/english/aeronomia.html -- 10.7 Кб -- 09.04.2016
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78. http://hea.iki.rssi.ru/conf/hea2010/Presentations/24/Titarchuk.pdf
... POWER SPECTRUM blue, red and black lines present power spectra of reprocessing function, pulsed signal and resulting pds respectively T, Laurent & shaposhnikov (2008) GK Per XMM Spectrum The XMM- Newton observation of GK Per on March 9 2002 (revolution 412) T, laurent & Shaposhnikov (2009) Red-skewed line in GK Per (CV) Relativistic interpretaion (CV) Ser X-1 Red skewed line in Cyg X-2. ... Soft state power spectrum of Cyg X-1 The composite soft state PDS is made by PCA (blue) and ASM (red) PDSs. ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2010/Presentations/24/Titarchuk.pdf -- 1854.0 Кб -- 26.01.2011
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79. 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? ...
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Ссылки http://www.gpad.ac.ru/collaborations/inasan.pdf -- 2655.7 Кб -- 05.07.2006
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80. Publications
... Archive of publications: . ... 2012 . 2011 . 2009 . 2008 . 2007 . 2006 . 2005 . 2004 . 2003 . ... From 2015 2014 2013 2012 2011 2009 2008 2007 2006 2005 2004 2003 to 2015 2014 2013 2012 2011 2009 2008 2007 2006 2005 2004 2003 . ... Solar System Research, Volume 40, Issue 4, pp.341-347, 2006. ...
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Ссылки http://www.tesis.lebedev.ru/en/publications.html?act=1&author=11& -- 14.1 Кб -- 11.04.2016
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Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
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