Team:Tokyo Tech/Ibuki test

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test<sup>[[#refrence|[1]]]</sup>
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<img src="https://static.igem.org/mediawiki/2009/8/89/Tokyotech.png" height="200">
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<a href="https://2009.igem.org/Team:Tokyo_Tech">Main</a>
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<a href="https://2009.igem.org/Team:Tokyo_Tech/Team">Team</a>
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<a href="https://2009.igem.org/Team:Tokyo_Tech/Project">Project</a>
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==refrence==
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*outside page[http://#]
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  <li><a href="https://2009.igem.org/Team:Tokyo_Tech/Iron-oxidizing">Iron-oxidizing bacteria</a></li>
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<table bordercolor=#000 border="1" width=960px><tr><td></td><tr></table>
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  <li><a href="https://2009.igem.org/Team:Tokyo_Tech/Consortium">Microbial consortium</a></li>
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  <li><a href="https://2009.igem.org/Team:Tokyo_Tech/Antifreeze">Antifreeze protein</a></li>
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  <li><a href="https://2009.igem.org/Team:Tokyo_Tech/Idea4">Idea 4</a></li>
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  <li><a href="https://2009.igem.org/Team:Tokyo_Tech/Idea5">Idea 5</a></li>
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</ul>
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<a href="http://partsregistry.org/cgi/partsdb/pgroup.cgi?pgroup=iGEM2009&group=Tokyo_Tech">Parts</a>
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<ul></ul></li>
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<a href="https://2009.igem.org/Team:Tokyo_Tech/Conclusion">Conclusion</a>
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<a href="https://2009.igem.org/Team:Tokyo_Tech/Links">Links</a>
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*アルベドと温度の関係について
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According to　Stefan-Boltzmann law,
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blackbody emit per surface in unit time is calculated as
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<!--<math>\sigma T^4</math>,-->
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&sigma;<i>T</i><sup>4</sup>,
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where T is the temperature of the black body and <math>\sigma=5.67*10^{-8} (W/m^2K^4)</math> is constant value.
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The total energy that comes from the sun is calculated as
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<!--<math>S(1-A)\pi r^2</math>,-->
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<i>S</i>(1 &minus; <i>A</i>)&pi;<i>r</i><sup>2</sup>,
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where <math>S=597 (W/m^2)</math>is the energy which actually reaches the mars from the sun,
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A is the albedo of the Mars and <math>r=3.3972*10^6 (m)</math> is the radius of the Mars.
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Regarding the Mars as blackbody, the radiative equilibrium temperature of the Mars is estimated as
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<math>T=\sqrt[4]{\frac{S(1-A)}{4\lambda}}</math>.
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According to Yurij Shkuratov and Larissa Starukhina, albedo A can be calculated as
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<math>A=\frac{1+\rho_b^2-\rho_f^2}{2\rho_b}-\sqrt{(\frac{1+\rho_b^2-\rho_f^2}{2\rho_b})^2-1}</math>,
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where <math>\rho_b</math> and <math>\rho_f</math> are the one-dimensional indicatrix back and forward.
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If we succeeded in decreasing the albedo by making the Mars black,
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the temperature will change as the graph shows.
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x axis is year and y axis is temperature.
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[[File:Temp.png|300px|thumb|temperature estimation]]
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If we could change the albedo from 0.15 to 0.05, the temperature of the Mars would increase by about 6 Celsius degree.
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Latest revision as of 19:12, 21 October 2009

Team photo

test[1]












refrence

  • outside page[http://#]
Retrieved from "http://2009.igem.org/Team:Tokyo_Tech/Ibuki_test"