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http://www.iki.rssi.ru/seminar/2011101821/presentation/Menshutin.pdf.
http://www.iki.rssi.ru/seminar/2011101821/presentation/Menshutin.pdf.
1. http://www.iki.rssi.ru/seminar/2011101821/presentation/Menshutin.pdf
... Particle starts at radius of birth Rbirth 3. ... If particles goes out of the radius of death Rdeath it is killed 6. ... D=3/2 (?) on the square lattice D=1.72 Off-lattice Problem definition · Large class of models of 2D growth results in similar structures (weakly speaking - "looks similar") · DLA model is the simplified model that captures main features of 2D critical aggregate growth · Scaling exponents are known only with 1% accuracy · Cluster behavior as N is still not understood · Multiscaling...
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Ссылки http://www.iki.rssi.ru/seminar/2011101821/presentation/Menshutin.pdf -- 819.6 Кб -- 07.11.2011
[ Текст ] Ссылки http://www.cosmos.ru/seminar/2011101821/presentation/Menshutin.pdf -- 819.6 Кб -- 07.11.2011
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[ Текст ] Ссылки http://www.cosmos.ru/seminar/2011101821/presentation/Menshutin.pdf -- 819.6 Кб -- 07.11.2011
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2. The AstroStat Slog particle physics
... Ah ha~ Once I questioned, ?what is systematic error?? (see [Q] systematic error. Thanks to L. Lyons? work discussed in [ArXiv] Particle Physics , I found this paper, titled Systematic Errors describing the concept and statistical inference related to systematic errors in the field of particle physics. ... Tags: coverage , Heinrich , likelihood , Lyons , nuisance parameter , objective priors , p-value , particle physics , statistical error , subjective priors , systematic error . ...
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Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/tag/particle-physics/index.html -- 26.0 Кб -- 01.03.2014
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3. Lecture Series 2010-2011 ? ?Particle Physics at the LHC and Cosmology? by
Lectures . ... Home Lectures Lecture Series 2010-2011 Lecture Series 2010-2011 ? Particle Physics at the LHC and Cosmology? by Michael Tuts . ... Lecture Series 2010-2011 . ... Beyond New York City . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... Amateur Astronomers Medal . ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...
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Ссылки http://www.aaa.org/lectures/lecture-series-2010-2011/lecture-series-2010-2011-particle-physics-at-the-lhc-and-cosmology-by-michael-tuts/ -- 99.5 Кб -- 10.04.2016
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4. Firtual Particles Are Not Only Particle Pairs - an Astronomy Net Blackholes2
Blackholes2 Forum Message . Forums: . ... Firtual Particles Are Not Only Particle Pairs . ... Posted by Richard Ruquist on October 19, 2004 12:03:20 UTC . ... Vacuum production of virtual particle pairs cannot violate the uncertainty principle. ... This theory is dual to the particle theory of gravitons. ... www.astronomy.net . About 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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Ссылки http://www.astronomy.net/forums/blackholes2/messages/4944.shtml -- 16.5 Кб -- 09.04.2016
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5. EDM (ImageJ API)
... public class EDM . ... Euclidean Distance Map: The value of each pixel is the distance to the nearest background pixel (for background pixels, the EDM is 0) - Ultimate Eroded Points (UEPs) are maxima of the EDM. ... static int . ... Unit in old make16bitEDM: this pixel value corresponds to a distance of one pixel. static int . ... int . ... For compatibility with previous versions of ImageJ only. public FloatProcessor makeFloatEDM ( ImageProcessor ip, int backgroundValue, boolean edgesAreBackground)...
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Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/plugin/filter/EDM.html -- 31.4 Кб -- 02.12.2010
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6. MONTE-CARLO
... COMPUTER SIMULATION OF RADIOWAVE MULTIPLE SCATTERING EFFECTS IN IONOSPHERE USING MONTE-CARLO METHOD . ... Distribution of reflected radiation on the ground is computed. ... Such influence can be remarkable if the scattering is multiple, i.e. the optical thickness for the scattering process is considerably greater than a unit. ... Radiation energy transfer in the slab is modeled by distribution of some particles carring small portions of radiation energy. ... The isotropic plasma approximation is...
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Ссылки http://ip.rsu.ru/~zabotin/posters/mont_car/mont_car.htm -- 12.8 Кб -- 02.02.2007
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7. Particle Sizes in Saturns Rings
... Particle Sizes in Saturns Rings . ... Credit: RSS , JPL , ESA , NASA Explanation: What size particles compose Saturn's rings? To help find out, the robot Cassini spacecraft now orbiting Saturn broadcast radio waves of three different wavelengths right through the rings to Earth earlier this month. The experiment was sensitive to ring particle sizes because ring particles much larger than a broadcast radio wavelength will reflect those radio waves away. ... NASA Official: Jay Norris. ...
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Ссылки http://www.astronet.ru/db/xware/msg/1205904 -- 14.0 Кб -- 25.05.2005
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8. Armagh Observatory
... Figure 4. (a) Ecliptic plane crossings; and (b) distribution of heliocentric distances, for sets of 1:3 Saturnian MMR and non-resonant Orionid particles in 450 A.D. Both sets of particles evolved dynamically for 2 kyr but the dense clustering of resonant meteoroids contrasts with the large dispersion of non-resonant particles. ... Many previous works have shown the relevance and dynamics of Jovian mean motion resonances (MMR) in various meteoroid streams. ...
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Ссылки http://star.arm.ac.uk/highlights/2013/633.html -- 5.5 Кб -- 17.05.2013
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9. 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
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10. Spherical particles
The classic solution for homogeneous sphere was suggested in 1899 by A.E.N. Love [ 330 ], in 1908 by G. Mie [ 342 ] and in 1909 by P. Debye [ 199 ]. ... Traditionally the theory of light scattering by a sphere is called the Mie theory. ... The exact solutions of the Mie problem for an optically active sphere (i.e. a sphere of optically active material [ 7 ]) and for a sphere with an optically active mantle were first obtained in 1974-5 by S. Bohren [ 158 , 159 ]. ...
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Ссылки http://www.astro.spbu.ru/DOP/3-REVS/KHLEB1/node4.html -- 7.6 Кб -- 19.11.2010
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11. The Beam Properties at the Distance of the Earth
... About ATNF overview . ... Parkes radio telescope . ... As a check on the properties of propagation in the turbulent field, we ran the program with a purely random field. ... In reaching the distance of the Earth from the Galactic Centre, a particle must travel through systematic fields which tend to deflect it away from the galactic plane. ... With our best model of the field and the position of the Earth, about one particle in one thousand reached the galactocentric distance of the Earth at . ...
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Ссылки http://www.atnf.csiro.au/pasa/17_3/clay2/paper/node3.html -- 55.2 Кб -- 08.04.2016
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12. C/2010 S1 (LINEAR), C/2010 R1 (LINEAR)
... Currently, there is very little information on comets which are active beyond the orbit of Jupiter. ... Previous observations conducted by our team with the SAO RAS 6-m telescope showed that some of these comets have extended tails dissimilar to the tails of comets forming at close heliocentric distances. ... We for the first time measured the linear polarization of scattered emission for the two distant comets C/2010 S1 (LINEAR) and C/2010 R1 (LINEAR) at heliocentric distances of 5.9-7.0 au. ...
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Ссылки http://www.sao.ru/Doc-en/SciNews/2015/Ivanova/ -- 5.7 Кб -- 10.04.2016
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13. How do scientists know that the particles revealed after a proton or lead ion
... How do scientists know that the particles revealed after a proton or lead ion collision are different from each other, such as quarks and muons, and not just smaller pieces of protons or lead ions? If I were to smash two lead bullets together, they would break into smaller pieces, but they would still be lead.) ... When particle accelerators collide protons or lead ions, they do so within special sections of an instrument that can capture fine details. ...
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Ссылки http://www.astronomy.com/magazine/ask-astro/2013/04/particles-after-collision -- 64.0 Кб -- 10.04.2016
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14. Phenomenology of particle acceleration in supernova remnants in the proximity
... Informazioni . Informazioni generali . ... Personale . Personale di Ricerca . Personale tecnico, amministrativo, bibliotecario . ... Personale in ordine alfabetico . ... Informazioni varie . Informazioni specifiche . ... Informazioni sindacali . ... Phenomenology of particle acceleration in supernova remnants in the proximity of molecular clouds - DD71/2015 . ...
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Ссылки http://www.arcetri.astro.it/home-italiano/218-gare-e-concorsi/concorsi-conclusi/967-2015-11-06-14-49-10 -- 33.7 Кб -- 10.04.2016
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15. ASP: Ghostly Particles All About
home publications > mercury . SEARCH ASP SITE: Match ALL words Match ANY word . ... Publications of the ASP (PASP) . ... Ghostly Particles All About . ... Rather than give up on this problem, Pauli?s imagination leaped in that darkness, and our understanding of Nature was propelled forward. ... Radioactivity refers to the process by which really big nuclei, which are made of large numbers of protons and neutral neutrons?like, say, nuclei of uranium or radium?rid themselves of excess energy. ...
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Ссылки http://www.astrosociety.org/pubs/mercury/35_01/ghostly.html -- 16.3 Кб -- 20.04.2012
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16. A New Stable Method for Long-Time Integration in an N-Body Problem
Next: Imaging by an Optimizing Method . ... A big advantage of this numerical integrator is its stability: the error in the semi-major axis and the eccentricity depends only on the step size and does not grow with an increasing number of time steps. ... As the integration time increases, the numerical results become more contaminated by various errors. ... A new symplectic integrator produces no secular truncation errors in the actions of a Hamiltonian system. ...
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Ссылки http://www.adass.org/adass/proceedings/adass96/taidakovat.html -- 9.4 Кб -- 23.06.1998
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17. Истомин Яков Николаевич (ФИАН)
... Acceleration of particles in the vicinity of a massive black hole We propose a two-step mechanism for charged particle acceleration in the magnetosphere of a massive black hole surrounded by an accretion disk. Particles first gain energy by stochastic process during the accretion phase. It is shown that effective proton acceleration up to energies eV is possible in the turbulent magnetized accretion disk. ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2007/abstracts/node28.html -- 5.3 Кб -- 19.12.2007
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18. http://astro.uni-altai.ru/AFgalleries.html
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Ссылки http://astro.uni-altai.ru/AFgalleries.html -- 1.1 Кб -- 01.10.2012
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19. The Satellite Telescope of Electrons and Protons STEP
The Satellite Telescope of Electrons and Protons STEP . ... Precision measurements of the energy, angular, and time distributions in precipitating fluxes of high-energy charged particles with solar, magnetospheric, and anomalous cosmic rays origin. ... Both "STEP-DI" and "STEP-DII" have an identical construction of large solid angle telescope from 4 detectors (D1-D4), first 2 of which (D1-D2) are position-sensitive silicon strip-detectors; both D3 and D4 are scintillation CsI(Tl) detectors. ...
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Ссылки http://space.univ.kiev.ua/projects/warning/step.html -- 8.5 Кб -- 15.02.2000
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20. 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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