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  • ...28&nbsp;000&nbsp;km, which lacks any visible structure like in the forward-scattering geometry.<ref name=Burns2004/><ref name=Showalter2005>{{cite conference |la ...alter2005/> However, larger bodies are required to explain the strong back-scattering and fine structure in the bright outer part of the main ring.<ref name=Burn ...
    40 KB (6,124 words) - 17:25, 21 July 2009
  • ...c radiation that are not generally referred to as "redshifts", including [[scattering]] and [[physical optics|optical effects]] (for more see section on [[#Effec ...e to such physical phenomena as [[Wolf effect|coherence effects]] or the [[scattering]] of [[electromagnetic radiation]] whether from [[electric charge|charged]] ...
    66 KB (9,812 words) - 16:59, 27 April 2010
  • [[Image:Electron-positron-scattering.svg|220px|thumb|right|A [[Feynman diagram]] of the exchange of a virtual ph | title = A Quantum Theory of the Scattering of X-rays by Light Elements ...
    86 KB (12,028 words) - 05:08, 13 August 2009
  • |title=High-Energy Inelastic ''e''–''p'' Scattering at 6° and 10° |title=Observed Behavior of Highly Inelastic Electron–Proton Scattering ...
    61 KB (8,771 words) - 19:12, 19 August 2009
  • ...through a process called [[Thomson scattering]]. Because of this repeated scattering, the early universe was opaque to light. ...atter when nearly all the electrons had recombined, at the ''epoch of last scattering'', 379,000 years after the Big Bang. These photons make up the CMB that is ...
    71 KB (10,449 words) - 08:42, 20 August 2009
  • ...y Wilkins ''et al.'', in 1953, for the ''in vivo'' B-DNA X-ray diffraction/scattering patterns of highly hydrated DNA fibers in terms of squares of [[Bessel func ...New York, 1962.</ref><ref>{{cite journal|author=Baianu, I.C. |title=X-ray scattering by partially disordered membrane systems.|journal=Acta Cryst., |volume=A34 ...
    95 KB (13,424 words) - 19:19, 3 February 2011
  • ...attered at an angle close to 180° (backwards) relative to solar light. The scattering angle is close to 90° for side-scattered light. ...
    29 KB (4,327 words) - 19:38, 16 August 2009
  • * [[Rayleigh scattering]] ...
    33 KB (4,583 words) - 16:34, 24 November 2010
  • In high mass main sequence stars, the opacity is dominated by [[electron scattering]], which is nearly constant with increasing temperature. Thus the luminosit ...
    49 KB (7,190 words) - 18:56, 4 June 2009
  • ...ing Outer Planets and Kuiper Belt: a)Before Jupiter/Saturn 2:1 resonance b)Scattering of Kuiper Belt objects into the solar system after the orbital shift of Nep ...
    58 KB (9,031 words) - 16:11, 18 August 2009
  • ...s seen in [[beer]] can be caused by clumps of [[protein]]s that [[Rayleigh scattering|scatter]] light.<ref>{{cite journal |author=Miedl M, Garcia M, Bamforth C | ...
    84 KB (12,734 words) - 06:55, 8 August 2009
  • ...g outer planets and Kuiper belt: a) Before Jupiter/Saturn 2:1 resonance b) Scattering of Kuiper belt objects into the Solar System after the orbital shift of Nep ...
    85 KB (12,829 words) - 17:09, 18 August 2009
  • ...g Outer Planets and Kuiper Belt: a) Before Jupiter/Saturn 2:1 resonance b) Scattering of Kuiper Belt objects into the solar system after the orbital shift of Nep ...
    83 KB (11,988 words) - 11:30, 20 August 2009
  • | title=The Scattering of α and β Particles by Matter and the Structure of the Atom | url=http://i ...
    94 KB (13,468 words) - 17:06, 20 August 2009