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  • [[Category:Crystallography/Lectures]] [[Category:Distances/Lectures]] ...
    8 KB (1,083 words) - 00:31, 28 January 2024
  • "Beyond the [[Solar System]] the distances in [[Radiation astronomy|astronomy]] are so great that using the au becomes {{main|Distances/Lengths|Lengths}} ...
    13 KB (2,045 words) - 04:58, 31 January 2020
  • ...he Federal Aviation Administration (FAA) requires aircraft to maintain set distances behind each other when they land. A joint NASA-FAA program aimed at boostin *[https://home.mpcdf.mpg.de/~bds/numerics/cfd-lectures.html Lectures on Computational Fluid Dynamics] ...
    4 KB (546 words) - 17:56, 25 March 2019
  • It is a lecture in a series about [[Special:Search |distances]]. Large distances are significant in astronomy. ...ion in a straight line, or rectilinear motion can be produced over limited distances in a laboratory, it may not occur naturally. ...
    17 KB (2,581 words) - 06:17, 31 January 2020
  • "In [[Draft:Keynote lectures/Radiation|radiation]] theory, the total number of light quanta is not const ...‘clouds’ of quark–antiquark excitations surrounding the electrons at short distances, modify the mixing of the photon and Z boson. This causes the effective wea ...
    13 KB (1,784 words) - 02:07, 30 April 2020
  • ...t area of the image may themselves be similar regions seen at much greater distances across the galaxy."<ref name=SpitzerSpaceTelescope/> [[Category:Abstractions/Lectures]] ...
    22 KB (3,213 words) - 02:22, 1 December 2020
  • ...' is an observational phenomenon that can be described in general terms of distances and times. {{main|Distances/Vectors|Vectors}} ...
    21 KB (3,274 words) - 04:42, 23 November 2020
  • '''The content of these notes is based on the lectures by [http://www.math.utah.edu/~milton/ Prof. Graeme W. Milton] (University o ...reated as a source of radiation. The change in phase due to the different distances traveled by the waves is then used to compute the intensity of the rainbow. ...
    12 KB (2,059 words) - 16:34, 25 February 2018
  • ...owave pulses that seemed to travel as much as 25% faster than c over short distances."<ref name=Glanz/> [[Category:Astrophysics/Lectures]] ...
    17 KB (2,630 words) - 02:31, 2 February 2020
  • * [[Keynote lectures/Dates|Dates]] (Hadean) (173 kB) (31 August 2019) * [[Draft:Distances]] (12 kB) (6 October 2019) ...
    16 KB (2,455 words) - 14:32, 23 December 2023
  • '''The content of these notes is based on the lectures by [http://www.math.utah.edu/~milton/ Prof. Graeme W. Milton] (University o ...terface shown in Figure 1. If the pressure is the same at points at equal distances from the interface as shown, the ...
    14 KB (2,212 words) - 11:01, 19 March 2024
  • |title=Electron Wavelength Data and Extinction Distances, In: ''Electron Microscopy of Thin Crystals'' ...ively weak on the subatomic scale. They are therefore able to travel great distances through matter without being affected by it. ...
    40 KB (5,854 words) - 02:53, 5 December 2020
  • ...ively weak on the subatomic scale. They are therefore able to travel great distances through matter without being affected by it. * [[Keynote lectures/Astrophysics|Astrophysics]] (106 kB) (7 July 2019) ...
    23 KB (3,348 words) - 05:40, 2 January 2021
  • * [[Keynote lectures/Dates|Dates]] (Hadean) (173 kB) (31 August 2019) * [[Draft:Distances|Distances]] (12 kB) (6 October 2019) ...
    42 KB (6,130 words) - 04:40, 16 December 2020
  • ...f.''' the "measurement of the diameters of heavenly bodies, their relative distances, etc."<ref name=HeliometryWikt>{{ cite book {{main|Distances/Radius/Sun|Solar radius}} ...
    39 KB (5,838 words) - 09:49, 30 May 2023
  • ...[logic]] (the trivium), along with [[arithmetic]], [[geometry]], [[Keynote lectures/Astronomy|astronomy]] and [[School:Music and Dance|music]] (the quadrivium) ...ate at the time of communication; thus communication can occur across vast distances in time and space. Communication requires that the communicating parties sh ...
    43 KB (5,978 words) - 02:21, 1 December 2020
  • |title=The extragalactic distance scale. IV - Distances of nearest groups and field galaxies from secondary indicators ...al stars (within 300 [[w:parsecs|parsecs]]) with [[w:Hipparcos|Hipparcos]] distances, and using numerical simulation, Charles Francis and Erik Anderson have cal ...
    38 KB (5,964 words) - 05:18, 18 December 2019
  • ...d allow two objects to affect each other’s behaviour instantly across vast distances".<ref name=Einstein>{{ cite journal ...rth is being continually and uniformly bombarded by cosmic [[Draft:Keynote lectures/Radiation|radiation]] at a rate evidently in excess of 10<sup>15</sup> cosm ...
    39 KB (5,700 words) - 00:23, 9 June 2022
  • ...imple autonomous vehicles using only low-level sensory information such as distances sensed by infra-red or sonar detectors. Each sensor is assumed to contribut * [[Keynote lectures/Detectors for radiation astronomy|Detectors for radiation astronomy]] (116 ...
    43 KB (6,339 words) - 09:34, 9 June 2021
  • "Red clump giants can provide a very precise estimate of the distances to metal-rich Galactic globular clusters and nearby galaxies."<ref name=Sta ...nge in peak absolute magnitude and can not be treated as standard candles. Distances to individual SNe II can be estimated by means of the expanding photosphere ...
    46 KB (6,963 words) - 22:28, 23 August 2021
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