Mikhail Koptev Yaroslav Mashtakov Mikhail Ovchinnikov Sergey Shestakov

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Mikhail Koptev Yaroslav Mashtakov Mikhail Ovchinnikov Sergey Shestakov 9th International Workshop on Satellite Constellations and Formation Flying, Boulder, CO, 19-21 June 2017 Novel Approach to Construction and Maintenance of Tetrahedral Formation Mikhail Koptev Yaroslav Mashtakov Mikhail Ovchinnikov Sergey Shestakov Keldysh Institute of Applied Mathematics, Moscow, Russia

Tetrahedral formation Earth’s magnetic field study, Space Research Institute of RAS Magnetospheric Multiscale Mission picture from www.nasa.gov 9th IWSCFF, Boulder, 19-21 June 2017

9th IWSCFF, Boulder, 19-21 June 2017 Problem statement Given four satellites on closed, possibly elliptical, orbits Need to obtain a reference orbit in order that the volume and shape of the corresponding tetrahedron maintain over time Size and shape must be formalized Also provide a control algorithm for several satellites to neglect perturbations 9th IWSCFF, Boulder, 19-21 June 2017

9th IWSCFF, Boulder, 19-21 June 2017 Problem statement Two satellites move passively along the same orbit The other two equipped with some control device e.g. magnetic attitude control system and thrusters 9th IWSCFF, Boulder, 19-21 June 2017

Tetrahedral configuration Quality of the tetrahedron Volume conservation is the conservation of the size Quality conservation is the conservation of the shape Quality is chosen to be meaningful in geometric sense and analytically analyzable 9th IWSCFF, Boulder, 19-21 June 2017

Reference orbit for circular motion Linearized HCW model, closed orbits estimation The main goal is to find such reference orbit that in passive motion in linearized model volume and quality of the tetrahedron remain constant 9th IWSCFF, Boulder, 19-21 June 2017

Reference orbit for circular motion Volume conserving conditions: relative orbits of controllable satellites must lie in parallel planes The reference orbit so that volume and quality of the tetrahedron conserve 9th IWSCFF, Boulder, 19-21 June 2017

9th IWSCFF, Boulder, 19-21 June 2017

Reference orbit for circular motion Volume and quality have the form This shape quality parameter achieves its maximal value when 9th IWSCFF, Boulder, 19-21 June 2017

9th IWSCFF, Boulder, 19-21 June 2017 Radius 10000 km, e=0, А=100 m and A=1000 m 9th IWSCFF, Boulder, 19-21 June 2017

Reference orbit for elliptic motion Solutions for corresponding linear model (TH equations) Make reference orbit analogous to circular one 9th IWSCFF, Boulder, 19-21 June 2017

Reference orbit for elliptic motion Parameters for reference orbit 9th IWSCFF, Boulder, 19-21 June 2017

Reference orbit for elliptic motion In this case quality has the form Choose coefficients A, B, and C, so that minimum over period be maximal 9th IWSCFF, Boulder, 19-21 June 2017

9th IWSCFF, Boulder, 19-21 June 2017 Pericenter 10000 km, apocenter 50000 km, e=0.66, А=100 m and A=1000 m, T = 14,5 h 9th IWSCFF, Boulder, 19-21 June 2017

9th IWSCFF, Boulder, 19-21 June 2017 Pericenter 10000 km, apocenter 100000 km, e=0.82, А=100 m and A=1000 m, T = 1,5 days 9th IWSCFF, Boulder, 19-21 June 2017

9th IWSCFF, Boulder, 19-21 June 2017 Pericenter 10000 km, apocenter 200000 km, e=0.9, А=100 m, T = 4 days 9th IWSCFF, Boulder, 19-21 June 2017

9th IWSCFF, Boulder, 19-21 June 2017 Pericenter 10000 km, apocenter 300000 km, e=0.94, А=100 m, T = 1 week 9th IWSCFF, Boulder, 19-21 June 2017

9th IWSCFF, Boulder, 19-21 June 2017 Pericenter 10000 km, apocenter 200000 km, e=0.9, А=100 m, T = 4 days 9th IWSCFF, Boulder, 19-21 June 2017

Two satellites control algorithm Pontryagin’s maximum principle Parallel shooting for boundary-value problem 9th IWSCFF, Boulder, 19-21 June 2017

Two satellites control in circular motion Quality degrading and compensation 20 passive revolutions 9th IWSCFF, Boulder, 19-21 June 2017

9th IWSCFF, Boulder, 19-21 June 2017 Conclusions The reference orbit for 4 sats conserving volume and shape of the tetrahedron is found in linear model on circular orbit For elliptic orbit the quality is periodic and conserves near the apocenter during several revolutions without any control Motion control (even in the case of single-axis control) allows to maintain a configuration (0.02 – 0,17 m/s/day depending on inclination) 9th IWSCFF, Boulder, 19-21 June 2017