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Mission Design for the CubeSat OUFTI-1

Mission Design for the CubeSat OUFTI-1

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CHAPTER 9where c p is <strong>the</strong> material’s heat capacity [ KJ ], k <strong>the</strong> conductivity [ W ], ⃗q <strong>the</strong>KgK mKheat flux and σ <strong>the</strong> energy generated inside <strong>the</strong> body.For a steady monodimentional problem without heat generation we have :⎧⎪⎨⎪⎩dqdx = −k d2 Tdx = 0T (0) = T 1T (L) = T 2(9.7)Solving <strong>the</strong> problem we have <strong>the</strong> following expression of <strong>the</strong> heat flux:Q 1→2 = qA = − T 2 − T 1LkAR eq = LkA(9.8)where A is <strong>the</strong> contact surface through which <strong>the</strong> heat can pass.As expected, <strong>the</strong> heat goes from <strong>the</strong> hotter body to <strong>the</strong> colder. We also have<strong>the</strong> expression of <strong>the</strong> equivalent conductive resistance.The same can be done <strong>for</strong> <strong>the</strong> radiation. With reference to figure 9.2, a bodyis in <strong>the</strong>rmal equilibrium with <strong>the</strong> heat flux Q , <strong>the</strong> irradiance G, <strong>the</strong> reflectedAirradiance G R and <strong>the</strong> radiant energy E.Figure 9.2: Equilibrium <strong>for</strong> radiative heat exchange{JA = Q + GAJ = E + G R = ɛE B + ρG = ɛE B + (1 − ɛ) G(9.9)where J is <strong>the</strong> radiosity and represent <strong>the</strong> total outgoing flux.We introduce <strong>the</strong> view factor F A,B , which represents <strong>the</strong> proportion of all <strong>the</strong>radiation which leaves surface A and strikes surface B <strong>for</strong> <strong>the</strong> first time, withoutmultiple reflection:Q 1→2 = F 1,2 A 1 (J 1 − J 2 ) (9.10)Galli Stefania 90 University of Liège

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