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Mission Design for the CubeSat OUFTI-1

Mission Design for the CubeSat OUFTI-1

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CHAPTER 8order to prevent any failure due to <strong>the</strong> switching it on and off, but we need toguarantee enough power. Fur<strong>the</strong>rmore, turning on and off <strong>the</strong> payload impliesthat commands have to be generated by <strong>the</strong> on-board computer or sent from<strong>the</strong> ground station.All <strong>the</strong> following analysis is made <strong>for</strong> <strong>the</strong> elliptic orbit in <strong>the</strong> hypo<strong>the</strong>sis of Ω = 0and ω = 0. However at <strong>the</strong> end of this chapter a parametric study <strong>for</strong> <strong>the</strong> powerproduced in orbit will be carry out making vary this two parameters: <strong>the</strong> resultsare basically <strong>the</strong> same but shifted in time and <strong>the</strong> most critical situation with<strong>the</strong> minimum power always happen. Fur<strong>the</strong>rmore, <strong>the</strong> orbital parameters aresupposed to remains constant.8.1 Eclipse’s durationThe first step to have an idea of <strong>the</strong> available power is to know <strong>the</strong> time ofeclipse: to have it, we need to know <strong>the</strong> direction of <strong>the</strong> sun rays on <strong>the</strong> orbitplane.As shown in figure 8.1, three planes play a role in this calculation with <strong>the</strong>irreference system: <strong>the</strong> ecliptic plane, <strong>the</strong> equator plane and <strong>the</strong> orbit plane.Figure 8.1: Reference sistemsAs shown in figure 8.1, <strong>the</strong> sun rays arrive to earth on <strong>the</strong> ecliptic plane on<strong>the</strong> direction:ˆN S = {cos (θ e ) sin {θ e } 0} (8.1)As above mentioned, <strong>the</strong> goal of this part is to express this direction into<strong>the</strong> orbit reference. We can trans<strong>for</strong>m a vector from <strong>the</strong> ecliptic plane into <strong>the</strong>equatorial plane thanks to a rotation about <strong>the</strong> x ecl = x eq with <strong>the</strong> <strong>the</strong> rotationmatrix R 1Galli Stefania 74 University of Liège

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