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21. http://www.ipa.nw.ru/conference/2002/sovet/PS/IVASHKIN.PS
... These trajectories have an initial flight from the Earth to a large distance (of about 1.5 million km), the following passive flight to the Moon's orbit, an approach to the Moon with a decrease of an energy of a particle (spacecraft) selenocentric motion to a negative value and the temporary capture in an elliptic orbit of the Moon's satellite. ... Several trajectories of this type are determined. ... Ivashkin V. V. On optimal trajectories of space flight to the Moon in the Earth--Moon--Sun system. ...
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Ссылки http://www.ipa.nw.ru/conference/2002/sovet/PS/IVASHKIN.PS -- 28.8 Кб -- 19.08.2002
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22. SOHO scientific payload
This is a subjective view on the sort of SOHO intruments and experiments. ... COSTEP (Comprehensive Suprathermal and Energetic Particle Analyzer), from the University of Kiel , Germany (in German). ... SUMER (Solar Ultraviolet Measurements of Emitted Radiation) . ... SUMER from GSFC , USA. ... GOLF (Global Oscillations at Low Frequencies), from the Institut d'Astrophysique Spatiale , France. ... MDI/SOI (Michelson Doppler Imager/Solar Oscillations Investigation), from Stanford University , USA. ...
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Ссылки http://crydee.sai.msu.ru/~vab/SohoInstr.htm -- 4.9 Кб -- 17.04.1997
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23. Laboratory of spectroscopy of defect structures ISSP RAS
... For SIMS (Secondary Ion Mass Spectrometry) analysis, a solid surface is bombarded by primary ions of some keV energy. ... The subsequent mass analysis of the emitted ions provides detailed information on the elemental and molecular composition of the surface. ... Extremely short ion pulses with a duration below . ... By rastering a fine-focussed ion beam over the surface, like an electron beam in an electron microprobe, mass resolved secondary ion images (chemical maps) can be obtained...
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Ссылки http://www.issp.ac.ru/lsds/en/methods/sims.html -- 10.6 Кб -- 10.04.2016
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24. CERN experiments observe particle consistent with long-sought Higgs boson |
... Tonight's Sky . ... Observing . ... Observing springtime deep-sky objects with a large telescope . ... CERN experiments observe particle consistent with long-sought Higgs boson . ... Just after the Tevatron collider at Fermilab in Illinois released its results , the Large Hadron Collider's (LHC) ATLAS and CMS experiment teams presented their latest preliminary results in the search for the long-sought Higgs particle at a seminar held at the European Organization for Nuclear Research (CERN) on July 4...
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Ссылки http://www.astronomy.com/en/Press%20Room/Press%20Releases/2012/09/~/link.aspx?_id=64BC1119D0AD4D9E854A059AA689807F&_z=z -- 70.3 Кб -- 10.04.2016
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25. Incoherent scatter
Previous page: How does a radar work? When the Arecibo incoherent scatter radar transmits into the ionosphere, each of the millions of electrons in the ionosphere illuminated by the beam acts as a very small target. The receiver sees a signal composed of the part of the sum total of all the reflections that falls on the 1000 foot dish. ... This tells us about the temperature in the ionosphere. (more on this on the next page) . The more electrons there are, the more power we receive. ...
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Ссылки http://www.naic.edu/~isradar/is/aboutis/incoherent_scatter.html -- 3.7 Кб -- 04.02.2000
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26. University Satellites and Space Science Education '2006
University Satellites and . Space Science Education . ... It is necessary to select a topic interesting from scientific point of view and simple enough to allow students understand and participate in all stages of experiment from measurements via data analysis to physical inference. ... Solar modulation effects and physical characteristics and analysis of the major solar events are possible only by joining data from space-born and surface particle and radiation detectors. ...
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Ссылки http://cosmos.msu.ru/universat2006/main.php?sec=reg&step=aview&id=1182&aid=921 -- 10.1 Кб -- 21.12.2007
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27. Measurement of the C/C Ratio in Planetary Nebulae
... The C III] multiplet near 1908? has a transition at 1909.6? completely forbidden in C, but allowed as a result of the non-zero nuclear spin of C. The C III] line was observed with the GHRS and Echelle-B and a positive detection of the C line was made in the Galactic C-rich PN NGC 3918; a marginal detection of the C line was made in SMC N2, which is also C rich. ... The derived C/ C ratio is 15 3. For SMC N2 the C line is much weaker and a 2 detection was made: the C/ C ratio was measured as 21. ...
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Ссылки http://www.stsci.edu/stsci/meetings/shst2/walshj2.html -- 19.0 Кб -- 15.06.2005
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28. The basic stages in the Earth's pre-geological development
... part 1 | ... The Basic Stages in Earth's Pre-geological Development . ... After fragments of the Vortex sleeves separated, whirlwinds of second and third orders ("NC" - new micro-vortex) were generated- future planet cores and their satellites - all of them developing independently, governed by the common laws of development of cosmogenic vortexes. ... Our planet's core today is comprised of considerably deteriorated cosmogenic vortex; consequently, the Earth has a moderated magnetic field. ...
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Ссылки http://www.lermus.ru/users/trunaev/part2.htm -- 22.6 Кб -- 04.12.2001
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29. Results of calculations
Next: Discussion Up: Old neutron star distribution Previous: Galactic potential . It proves to be teachful to have a look at the calculated distribution (Fig. ... The galactic z -distribution of stars and peculiar velocities slightly smear out this narrow boundary. ... The final picture (Fig. ) of the old neutron star density distribution is obviously the sum of filled equipotential lobes with different weighted with the probability shown in the Fig. ...
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Ссылки http://xray.sai.msu.ru/~mystery/articles/old_ns/node9.html -- 6.0 Кб -- 19.08.1996
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30. Mark 2 Consciousness
P.O. Box 797 Sonoita, AZ 85637-0797 June 19, 2000 Prof. David Chalmers Philosophy Department Room 213, Social Sciences Building University of Arizona Tucson, AZ 85721-0027 Dear Prof. Chalmers: Well, here's another one from Mr. At-Least-I-Thought-Of-It-Independently. ... So as a thought experiment, let's imagine that instead of having our matter transporter actually move matter, what it moves is information. ... That will make it necessary to move the matter to move consciousness. ...
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Ссылки http://www.winer.org/About/cons_mark_2.html -- 6.6 Кб -- 27.02.2014
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31. http://www.mso.anu.edu.au/~agris/Larry/ReadMe
... The forces of the mobile are calculated using a grid scheme. ... The initial parameters are coded in the file names: The number after Speed is the pattern speed of the initial quadrupole field and frac is the fraction of disk particles . [agris@mizar ~/ Mar ]# ll ~/public_html/Larry/ 6033838 Mar 2 10:14 Speed -0.08- frac -0.0g.ps 6035344 Mar 2 10:14 Speed -0.08- frac -0.1g.ps 6040839 Mar 2 10:14 Speed -0.16- frac -0.0g.ps 8778756 Mar 2 10:14 ...
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Ссылки http://www.mso.anu.edu.au/~agris/Larry/ReadMe -- 4.6 Кб -- 02.03.2007
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32. Spectral energy distribution
... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...
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Ссылки http://mavr.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 02.10.2012
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 01.10.2012
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[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 01.10.2012
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33. Astronaut Bio: James P. Bagian (05/1995)
... James P. Bagian (M.D., P.E.) . ... SPECIAL HONORS: U.S. Army ROTC Superior Cadet Award (1970); graduated first in class from Drexel University (1973); Orthopedics Prize from Jefferson University (1977); Honor Graduate (first in class) from USAF Flight Surgeons School (1979); Federation Aeronautique Internationale (FAI) Komarov Diploma (1989); Sikorsky Helicopter Rescue Award (1990); NASA Achievement Award for developing treatment of space motion sickness (1991); NASA Space ...
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Ссылки http://www.jsc.nasa.gov/Bios/htmlbios/bagian.html -- 10.1 Кб -- 07.07.2015
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34. http://master.sai.msu.ru/static/YaB_100/20/Khlopov.pdf
... 20 , 2014, , Outlines · Cosmological impact of new stable particles: direct and indirect searches for dark matter · Cosmological patterns of particle symmetry breaking: archioles, massive PBH clusters, antimatter domains . ... They are: · Inflation · Baryosynthesis · Dark matter/energy All these phenomena imply extension of the Standard Model of Strong (QCD) and Electroweak Interactions. ... Dark Matter from Charged Particles? ... Advances in High Energy Physics, vol. ...
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Ссылки http://master.sai.msu.ru/static/YaB_100/20/Khlopov.pdf -- 1073.1 Кб -- 08.04.2014
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35. radiazpe
The radiation belts around the planets are the interrnal regions of planets' magnetospheres where the own magnetic field of a planet keeps the charged particles (protons and electrons) having the great kinetic energy. ... They usually distinguish the Earth's internal and external radiation belts. the internal radiation belt of the Earth has the maximum particles density (mainly protones) over the equator in the height of 22 thousand km. ... Jupiter and Saturn have the powerful radiation belts. ...
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Ссылки http://www.space.vsi.ru/radiazpe.htm -- 2.1 Кб -- 14.10.2000
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36. Cosmic Rays at Ground Level
... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... Cosmic Ray Induced Noise in Gravitational Wave Detectors . ... In effect then, all ground level cosmic rays are secondaries resulting either from the first interaction or from a cascade of secondaries (an extensive air shower, or EAS). ...
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Ссылки http://www.atnf.csiro.au/pasa/14_2/clay/paper/node2.html -- 54.0 Кб -- 08.04.2016
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37. Blowin' in the wind: both `negative' and `positive' feedback in an obscured
... Galaxies, AGN, Cosmology . ... Blowin' in the wind: both `negative' and `positive' feedback in an obscured high-z Quasar . ... However, finding observational evidence of the effect of such AGN negative and positive feedback is still one of the main challenges in extragalactic astronomy . ... The results of this work are presented in the article " Blowin' in the wind: both `negative' and `positive' feedback in an obscured high-z Quasar ", Astrophysical Journal (in press; arXiv:1411.4208 ) . ...
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Ссылки http://www.arcetri.astro.it/en/previous/204-scientific-news/795-qso-positive-feedback -- 32.1 Кб -- 10.04.2016
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38. Подлипнов Владимир Владимирович. Публикации
... Информация Руководство и преподаватели Подлипнов Владимир Владимирович . ... Публикации . ... Kolpakov V.A. , Podlipnov V.V. Mechanism of interaction between a directed beam of negative particles from a gas-discharge plasma and the melted nickel surface // Technical Physics. ... Kazanskiy N.L. , Kolpakov V.A. , Podlipnov V.V. Gas discharge devices generating the directed fluxes of off-electrode plasma // Vacuum. 2014. ... Podlipnov. ... 846) 335-18-26 Факс: (846) 335-18-36 . ...
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Ссылки http://www.ssau.ru/staff/131487205-Podlipnov-Vladimir-Vladimirovich/publ -- 19.9 Кб -- 27.04.2015
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39. East Siberian Center for the Earth's Ionosphere Research. Ionospheric parameter
Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Investigations of the ionospheric response to strong magnetics storms which are usual for our latitudes, are of great interest. ... In the figure, we present ionospheric parameter dynamics during three perturbed days in July 2000. ...
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Ссылки http://rp.iszf.irk.ru/esceir/isr/vozmnr2en.htm -- 3.9 Кб -- 04.06.2001
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40. Basic CCD image processing
... These are the typical steps through which a CCD image has to go. ... That process is repeated until all the pixels from the 1st line are read out. ... Figure 1: raw CCD image, obtained with a Tektronics 1024; refer to the bottom of the page for the technical details. ... The corresponding raw image presents all the defects and artifacts of the CCD and the telescope. ... These are the most basic steps; every image published should have received the following corrections. ... IfA Hale-Bopp page | ...
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Ссылки http://www.eso.org/~ohainaut/ccd/ -- 11.4 Кб -- 18.08.2004
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