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1. The Motion of Magnetically Trapped Particles -- History
... Files in red?history) . ... Trapped Motion . ... 10a. Particle Drift . ... Fast Particles . ... The fact charged particles circle around field lines was well known to J.J. Thomson when he experimented with electron and ion beams in a magnetic field. ... The notion of adiabatic invariance is tied with the early years of quantum theory. ... By about1910, physicists realized that these patterns indicated changes in the laws of physics as one approached atomic dimensions. ...
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/mirrors/stern/Education/whtrap2.html -- 11.9 Кб -- 24.03.2006
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2. The Motion of Magnetically Trapped Particles -- History
... Files in red?history) . ... Trapped Motion . ... 10a. Particle Drift . ... Fast Particles . ... The fact charged particles circle around field lines was well known to J.J. Thomson when he experimented with electron and ion beams in a magnetic field. ... The notion of adiabatic invariance is tied with the early years of quantum theory. ... By about1910, physicists realized that these patterns indicated changes in the laws of physics as one approached atomic dimensions. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/mirrors/stern/Education/whtrap2.html -- 11.9 Кб -- 21.12.2007
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3. As I Understand Virtual Paticles - an Astronomy Net Blackholes2 Forum Message
Blackholes2 Forum Message . Forums: . ... As I Understand Virtual Paticles . ... Posted by Duane Eddy on October 19, 2004 03:40:44 UTC . ... Firtual particles are not only particle pairs - yanniru - October 19, 2004 - 12:03 UTC . Faster then light travel? - duordi - October 19, 2004 - 20:53 UTC . ... 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" . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/forums/blackholes2/messages/4943.shtml -- 16.4 Кб -- 09.04.2016
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4. http://zebu.uoregon.edu/tandf/toc.html
... 2.3 Establishing the Extragalactic Distance Scale . ... 2.3.2 The Second Rung: Distances to stellar clusters . ... 2.3.4 Distances to Local Group Galaxies . ... The Luminosity Function of Planetary Nebulae . ... 3.2.2 Clusters of Galaxies . ... 4.2 Evidence for Dark Matter as a Function of Scale Size . ... 4.3 Other Dark Matter Indicators for Galaxies . ... What is the nature of the large-scale distribution of matter in the universe as traced by the three-dimensional galaxy distribution? ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/tandf/toc.html -- 10.7 Кб -- 17.07.1998
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5. A Particle Beam Jet forms HH 24
... A Particle Beam Jet forms HH 24 . ... Credit Copyright: Hubble Legacy Archive , NASA , ESA - Processing: Judy Schmidt Explanation: If you visit HH 24, don't go near the particle beam jet. ... The above image was taken by the Hubble Space Telescope in infrared light in order to better understand turbulent star forming regions known as Young Stellar Objects (YSOs). Frequently when a star forms, a disk of dust and gas circles the YSO causing a powerful central jets to appear. ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/1299792 -- 14.9 Кб -- 04.02.2014
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6. Research Interests
... 12) Das, S., Becker, P. A. Le, T. " Dynamical Structure of Viscous Accretion Disks with Shocks ," 2009, Vol 702, page 649. ... 921, Page 462. ... 6) Le, T. , Becker, P. A., " Particle Acceleration in Advection-Dominated Accretion Disks with Shocks: Green's Function Energy Distribution ," 2007, ApJ, Vol. 661, page 416. ... 4) Le, T. , Becker, P. A., " Particle Acceleration and the Production of Relativistic Outflows in Advection-Dominated Accretion Disks with Shocks ," 2005, ApJ, Vol. 632, page 476. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~tle/ -- 11.5 Кб -- 28.05.2010
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7. Armagh Observatory
... Armagh Observatory, 14th August 2015: Armagh ObservatoryтАЩs Leverhulme Postdoctoral Researcher Dr Maria Madjarska, who has been working for the last two years with the ObservatoryтАЩs head of solar physics, Professor Gerry Doyle, has recently received a grant from the Royal Society to develop a new interdisciplinary project aimed at improving understanding of how changes in the SunтАЩs activity affect EarthтАЩs near-space environment and hence conditions here on Earth . ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/press/2015/weather_research_grant_pr.html -- 9.1 Кб -- 13.08.2015
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8. 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 . ...
[ Сохраненная копия ]  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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9. APOD: 2003 June 23 - KamLAND Verifies the Sun
... 2003 June 23 . KamLAND Verifies the Sun . Credit: KamLAND Collaboration . Explanation: A large sphere beneath Japan has helped verify humanity's understanding of the inner workings of the Sun . ... KamLAND 's results bolster previous neutrino oscillation claims including that from the Sudbury detector , a similar large sphere beneath Canada designed to detect all types of neutrinos from the Sun . ... About APOD | ... NASA Web Site Statements, Warnings, and Disclaimers . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap030623.html -- 5.4 Кб -- 02.10.2012
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10. 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. ...
[ Сохраненная копия ]  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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11. Wavelength dependence
... The first task assumes the searching for chemical composition and sizes of particles which give the wavelength dependence of the extinction efficiencies close to the observed dependence of . Figure 7: Wavelength dependence of the extinction efficiency factors for homogeneous spherical particles of different sizes consisting of astronomical silicate and amorphous carbon. The dashed segment shows the approximate wavelength dependence of the mean galactic extinction curve at optical wavelengths. ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/DOP/8-GLIB/ASTNOTES/node3.html -- 15.8 Кб -- 19.11.2010
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12. Understanding Infrared emission from galaxies Bojan Nikolic web pages (r. 329)
... Bojan Nikolic web pages (r. 329) . Modelling absorption and emission of radiation by interstellar dust . ... The search results are restrict to these pages only . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/ir/index.html -- 7.4 Кб -- 04.04.2016
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13. Understanding UNIX files
Files do not actually reside inside directories. ... The directory holds two pieces of information about each file: . ... an inode number which acts as a pointer to where the system can find the information it needs about this file. Filenames are only used by the system to locate a file and its corresponding inode number. ... To the system, the file is the inode number. Multiple filenames can be used to refer to the same file by creating a link between an inode and each of the filenames. ...
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/UNIXhelp/concepts/file.html -- 2.3 Кб -- 17.01.1997
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14. http://www.naic.edu/~astro/talks/abstracts/chu_18apr05.htm
... Pole-To-Pole" LIDAR "Expedition" for Middle Atmosphere Study . Human induced changes in the global climate and atmospheric environment are among the most significant scientific challenges of this century. ... Models of the global atmosphere are used to understand these issues and to project the future state of the climate and the environment. ... These results show examples how the lidar observations can contribute to the tests of large-scale dynamics in atmospheric models. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~astro/talks/abstracts/chu_18apr05.htm -- 3.9 Кб -- 13.04.2005
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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. ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/pubs/mercury/35_01/ghostly.html -- 16.3 Кб -- 20.04.2012
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16. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B26394131-4168-4273-AC85-B815F210AA32%7D
. A "radio phoenix" has been discovered using X-ray, radio, and optical data. This system contains the collision of two galaxy clusters located about 1.6 billion light years from Earth. The collision re-energized a regeneration of vast clouds of high-energy particles that primarily radiate at radio frequencies. Understanding how galaxy clusters grow over time, including through collisions, is important for cosmology. X-ray: NASA/CXC/Univ of Hamburg/F. de Gasperin et al; Optical: SDSS; Radio: NRAO/VLA
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B26394131-4168-4273-AC85-B815F210AA32%7D -- 3.8 Кб -- 10.04.2016
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17. http://www.atnf.csiro.au/research/Astro2010/talks/mverdon.pdf
Pulsar radio emission - oscillating model M. Verdon, D. Melrose University of Sydney 10 th June, 2010 Outline Problems understanding pulsar radio emission Magnetosphere model Emission mechanisms Oscillating model Wave modes Time-dependence Coupling What is a pulsar? rotation axis magnetic axis polar cap open field line region closed field line region Emission models Production of ...
[ Текст ]  Ссылки http://www.atnf.csiro.au/research/Astro2010/talks/mverdon.pdf -- 553.5 Кб -- 16.06.2010
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18. Towards a better understanding of AGN
Paolo Padovani . Original Version: `New Horizons from Multi-Wavelength Sky Surveys', B. McLean et al. eds., p. 257. ... Active Galactic Nuclei (AGN) are ideal sources for multi-wavelength studies as their emission can cover almost 20 orders of magnitude in frequency from the radio to the gamma-ray band. ... I will then briefly illustrate how currently available and forthcoming sky surveys will help in addressing some of the open questions of AGN studies. ... Figure 1 (65kb) . Figure 2 (23kb) . ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~ppadovan/multi.html -- 3.1 Кб -- 10.08.2004
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19. Lunar Prospector
... NASA Lunar Orbiter . ... The Lunar Prospector is designed for a low-polar orbit investigation of the Moon, including mapping of surface composition and possible polar ice deposits, measurements of magnetic and gravity fields, and study of lunar outgassing events. Data from the 1- to 3-year mission will allow construction of a detailed map of the surface composition of the Moon, and will improve our understanding of the origin, evolution, current state, and resources of the Moon. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/solar/eng/lunpros.htm -- 5.2 Кб -- 15.10.1997
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/Astro/solar/eng/lunpros.htm -- 6.0 Кб -- 15.03.1998
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20. http://www.mccme.ru/dubna/2015/notes/simon-notes.pdf
... In this context, finding the equilibrium value of macroscopic variables (like temperature) amounts to computing a probability distribution. Such a probability law depends on a finite number of parameters, and describes the possible states of the system composed of a huge amount of particles. ... This is done with the help of a few macroscopic variables such as the internal energy E, the volume V, the pressure P, the number of particles N, the temperature T, the entropy S, and others. ...
[ Текст ]  Ссылки http://www.mccme.ru/dubna/2015/notes/simon-notes.pdf -- 207.6 Кб -- 21.07.2015
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