Changes between Version 3 and Version 4 of gallery/movies/cbl


Ignore:
Timestamp:
Dec 12, 2012 10:35:57 AM (12 years ago)
Author:
maronga
Comment:

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  • gallery/movies/cbl

    v3 v4  
    148148
    149149
    150 ||||='''Fifth sequence: structure parameter for temperature C,,T,,^2^ (2010)''' =||
     150||||='''Fifth sequence: dust devils in the convective boundary layer (2012)''' =||
     151{{{#!td style="vertical-align:top; border: 0px solid"
     152{{{#!html
     153<embed
     154    type="application/x-shockwave-flash"
     155    id="player"
     156    name="player"
     157    src="http://palm.muk.uni-hannover.de/chrome/site/gallery/player.swf"
     158    width="512"
     159    height="293"
     160    allowfullscreen="true"
     161    flashvars="file=http://palm.muk.uni-hannover.de/chrome/site/gallery/movies/dd_flash.flv&image=http://palm.muk.uni-hannover.de/chrome/site/gallery/movies/dd_preview.png"
     162/>
     163}}}
     164}}}
     165{{{#!td style="vertical-align:top; border: 0px solid""
     166'''Responsible:''' [[imuk/members/hoffmann|Fabian Hoffmann]], [[imuk/members/maronga|Björn Maronga]]\\
     167\\
     168'''Project:''' [[imuk/projects/2011_01|Numerical impacts on the strength of simulated dust devils]]\\
     169\\
     170'''Description:''' \\
     171This sequence shows the development of a large dust devil during a time period of 10 minutes. The shown region has a horizontal extent of 350 m x 300 m and is about 300 m high. The dust devil is made visible by a passive scalar which is advected by the flow. The surface flux of the passive scalar is calculated by a simple parametrization of the saltation process which depends on the friction velocity (White, 1979). Due to uncertainties in the parametrization of the surface flux, the displayed concentrations of the passive scalar are in arbitrary units. Dust concentrations in the order of magnitude of 0.1 g/m3 have been found for dust devils in field measurements (Renno et al., 2004).
     172\\
     173
     174||||='''Model Setup'''  =||
     175||Total domain size (x|y|z):||768m x 768m x 945m||
     176||Grid spacing (x|y|z):||1m x 1m x 1m||
     177||Number of grid points (x|y|z):||768 x 768 x 832||
     178||Simulated time:||3h||
     179||CPU-time:||24h||
     180||Number of CPUs:||2048||
     181||Machine/ processor type:||SGI Altix ICE at HLRN||
     182||Visualization software:||VAPOR||
     183\\
     184}}}
     185
     186
     187\\
     188
     189
     190
     191||||='''Sixth sequence: structure parameter for temperature C,,T,,^2^ (2010)''' =||
    151192{{{#!td style="vertical-align:top; border: 0px solid"
    152193{{{#!html
     
    182223\\
    183224}}}
    184 
    185 
    186 \\
    187 
    188 
    189 ||||='''Sixth sequence: dust devils in the convective boundary layer (2012)''' =||
    190 {{{#!td style="vertical-align:top; border: 0px solid"
    191 {{{#!html
    192 <embed
    193     type="application/x-shockwave-flash"
    194     id="player"
    195     name="player"
    196     src="http://palm.muk.uni-hannover.de/chrome/site/gallery/player.swf"
    197     width="512"
    198     height="293"
    199     allowfullscreen="true"
    200     flashvars="file=http://palm.muk.uni-hannover.de/chrome/site/gallery/movies/dd_flash.flv&image=http://palm.muk.uni-hannover.de/chrome/site/gallery/movies/dd_preview.png"
    201 />
    202 }}}
    203 }}}
    204 {{{#!td style="vertical-align:top; border: 0px solid""
    205 '''Responsible:''' [[imuk/members/hoffmann|Fabian Hoffmann]], [[imuk/members/maronga|Björn Maronga]]\\
    206 \\
    207 '''Project:''' [[imuk/projects/2011_01|Numerical impacts on the strength of simulated dust devils]]\\
    208 \\
    209 '''Description:''' \\
    210 This sequence shows the development of a large dust devil during a time period of 10 minutes. The shown region has a horizontal extent of 350 m x 300 m and is about 300 m high. The dust devil is made visible by a passive scalar which is advected by the flow. The surface flux of the passive scalar is calculated by a simple parametrization of the saltation process which depends on the friction velocity (White, 1979). Due to uncertainties in the parametrization of the surface flux, the displayed concentrations of the passive scalar are in arbitrary units. Dust concentrations in the order of magnitude of 0.1 g/m3 have been found for dust devils in field measurements (Renno et al., 2004).
    211 \\
    212 
    213 ||||='''Model Setup'''  =||
    214 ||Total domain size (x|y|z):||768m x 768m x 945m||
    215 ||Grid spacing (x|y|z):||1m x 1m x 1m||
    216 ||Number of grid points (x|y|z):||768 x 768 x 832||
    217 ||Simulated time:||3h||
    218 ||CPU-time:||24h||
    219 ||Number of CPUs:||2048||
    220 ||Machine/ processor type:||SGI Altix ICE at HLRN||
    221 ||Visualization software:||VAPOR||
    222 \\
    223 }}}