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University of Paderborn Applied Mathematics Michael Dellnitz Albert Seifried Applied Mathematics University of Paderborn Energetically efficient formation flight of spacecraft: numerical experiments Jens Levenhagen Astrium GmbH Oliver Junge Applied Mathematics University of Paderborn
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Applied Mathematics Motivation NASA: Terrestrial Planet Finder ESA: Darwin
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University of Paderborn Applied Mathematics Table of Contents 1.Computing the deformation of a spacecraft formation under the natural dynamics (globally) 2.Computing the deformation along Halo orbits 3.Controlling the formation on a Halo orbit
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University of Paderborn Applied Mathematics circular restricted three body problem rotating coordinates 3D flow: L4L4 L3L3 L5L5 L1L1 L2L2 The model
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University of Paderborn Applied Mathematics Computing the deformation* Compute the deformation of tetrahedra under evolution of their vertices: *related approach for near earth formations: W. Koon, J. E. Marsden, J. Masdemont, and R. M. Murray. J2 dynamics and formation flight, Proceedings of AIAA Guidance, Navigation, and Control Conference, Montreal, Canada, August, AIAA 2001 deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Computing the deformation Consider a partition of part of the phase space into boxes: L2L2 In every box B compute the average over the deformation of n tetrahedra: deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Deformation globally time of integration: ca. 8 months length of the edges: 150m – 1.5 km deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Deformation near the Earth deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Deformation near L 2 L2L2 deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Deformation near L 2 in dependence of T deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Observations there is no region where the deformation always vanishes; there are regions where the deformation regularily grows and shrinks again; typically in these regions the deformation is high only for a short period of time („peaks“). T Def(.,T) deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Deformation averaged over time deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Trajectory with low time-averaged deformation L2L2 L2L2 L2L2 deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Maximal deformation within [0,T] deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Solution with low maximal deformation L2L2 deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Halo-Orbits L2L2 Sun deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Deformation along Halo-Orbits deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Deformation along Halo-Orbits (adapted initial velocity) deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Controlled formation flight Model: additive force in each space direction. Control for each spacecraft (j=1,...,4): from current point q j (t i ) (configuration space) reach prescribed point q j (t i+1 ), i.e. solve h : stepsize, u i R 3 : control. deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Results for a Halo orbit near L 2 distances between actual and target vertices: meter months deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Results for a Halo orbit near L 2 norm of controls: N/kg months deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Results for a Halo orbit near Earth distances between actual and target vertices: meter months deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Results for a Halo orbit near Earth norm of controls: N/kg months deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Transition to a local coordinate system Observation: scales differ by a factor of 10 13 : distance Sun-Earth: 1.5·10 11 m maximal error for distances between spacecraft: 0.01 m rounding effects start to play a role But: machine precision („ double “): 10 -16 Idea: transition to a local coordinate system origin: center of mass of the formation origin evolves on Halo-orbit dynamics of the formation according to the linearized dynamics (variational equation along Halo-orbit) distances between actual and target vertices: meter months deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Results for the linearized model distances between actual and target vertices: meter months deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Results for the linearized model norm of controls: N/kg months deformation globally deformation along Halos controlling the formation
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University of Paderborn Applied Mathematics Outlook replace „reach exact target vertex“ by a more flexible target configuration: allow for rotation around normal allow for maximal error in distances between the spacecraft locally optimal control of formation compute globally optimal control using Bellman´s principle application of NTG?
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