768 research outputs found

    Comprehensive review on controller for leader-follower robotic system

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    985-1007This paper presents a comprehensive review of the leader-follower robotics system. The aim of this paper is to find and elaborate on the current trends in the swarm robotic system, leader-follower, and multi-agent system. Another part of this review will focus on finding the trend of controller utilized by previous researchers in the leader-follower system. The controller that is commonly applied by the researchers is mostly adaptive and non-linear controllers. The paper also explores the subject of study or system used during the research which normally employs multi-robot, multi-agent, space flying, reconfigurable system, multi-legs system or unmanned system. Another aspect of this paper concentrates on the topology employed by the researchers when they conducted simulation or experimental studies

    Advances in Spacecraft Systems and Orbit Determination

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    "Advances in Spacecraft Systems and Orbit Determinations", discusses the development of new technologies and the limitations of the present technology, used for interplanetary missions. Various experts have contributed to develop the bridge between present limitations and technology growth to overcome the limitations. Key features of this book inform us about the orbit determination techniques based on a smooth research based on astrophysics. The book also provides a detailed overview on Spacecraft Systems including reliability of low-cost AOCS, sliding mode controlling and a new view on attitude controller design based on sliding mode, with thrusters. It also provides a technological roadmap for HVAC optimization. The book also gives an excellent overview of resolving the difficulties for interplanetary missions with the comparison of present technologies and new advancements. Overall, this will be very much interesting book to explore the roadmap of technological growth in spacecraft systems

    A comparative study of the extended Kalman filter and sliding mode observer for orbital determination for formation flying about the L(2) Lagrange point

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    Two nonlinear state estimation techniques, the Sliding Mode Observer and the Extended Kalman Filter, are compared in terms of their ability to provide accurate relative position and velocity estimates for a formation flying mission about the Earth/Moon - Sun L2 libration point. The observers are individually tested on the NASA Constellation X simulation model. Constellation X is a proposed x-ray telescope mission, where formation flying spacecraft was considered as a possible mission scenario. A follower spacecraft is controlled to maintain a fixed distance (50 meters) from a leader spacecraft to with 1 millimeter accuracy. The state estimates propagated by each observer were of sufficient accuracy to maintain the required separation distance to within mission design requirements. For these particular formations of the Extended Kalman Filter and the Sliding Mode Observer, the Extended Kalman Filter is shown to be less sensitive to measurement noise levels, and the Sliding Mode Observer is shown to be less sensitive to input disturbances. There is no overall significant difference in sensitivity to parametric uncertainties between observers

    ํ•ด๋ฐ€ํ„ด ๊ตฌ์กฐ์™€ ์™ธ๋ž€ ๊ด€์ธก๊ธฐ ๊ธฐ๋ฒ•์„ ์ด์šฉํ•œ ๋ผ๊ทธ๋ž‘์ฃผ ์  ๊ถค๋„ ์ฃผ๋ณ€์—์„œ์˜ ๊ฒฝ๊ณ„ ์ƒ๋Œ€ ์šด๋™ ๋ฐ ๊ถค๋„์œ ์ง€

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    ํ•™์œ„๋…ผ๋ฌธ (๋ฐ•์‚ฌ) -- ์„œ์šธ๋Œ€ํ•™๊ต ๋Œ€ํ•™์› : ๊ณต๊ณผ๋Œ€ํ•™ ๊ธฐ๊ณ„ํ•ญ๊ณต๊ณตํ•™๋ถ€, 2020. 8. ๊น€์œ ๋‹จ.In this dissertation, a novel strategy for station-keeping and formation flight of spacecraft in the vicinity of unstable libration point orbits is presented, and its performance and stability are analyzed. The presented control strategy leverages the Hamiltonian nature of the equations of motion, rather than simply applying the control theory from the perspective of ``signal processing". A filtered extended high-gain observer, a kind of disturbance observer, is designed to mitigate the performance degradation of the control strategy due to model uncertainties and external disturbances. Canonical coordinates are adopted to design a controller that exploits the mathematical structure of Hamiltonian system inherent in orbital mechanics, and then the equations of motion of spacecraft are represented in the form of Hamilton's equation with generalized coordinates and momenta. The baseline controller, utilizing the canonical form of the Hamiltonian system, is divided into two parts: i) a Hamiltonian structure-preserving control, and ii) an energy dissipation control. Hamiltonian structure-preserving control can be designed in accordance with the Lagrange-Dirichlet criterion, i.e., a sufficient condition for the nonlinear stability of Hamiltonian system. Because the Hamiltonian structure-preserving control makes the system marginally stable instead of asymptotically stable, the resultant motion of the Hamiltonian structure-preserving control yields a bounded trajectory. Through the frequency analysis of bounded relative motion, a circular motion can be achieved for particular initial conditions. By appropriately switching the gain of the Hamiltonian structure-preserving control, the radius of bounded motion can be adjusted systematically, which is envisioned that this approach can be applied to spacecraft formation flight. Furthermore, the energy dissipation control can be activated to make the spacecraft's bounded relative motion converge to the nominal orbit. On the other hand, a filtered extended high-gain observer is designed for the robust station-keeping and formation flight even under highly uncertain deep-space environment. The filtered extended high-gain observer estimates the velocity state of the spacecraft and disturbance acting on the spacecraft by measuring only the position of the spacecraft. The filtered extended high-gain observer includes an integral state feedback to attenuate navigation error amplification due to the high gain of the observer. The global convergence of the observer is shown, and it is also shown that the tracking error is ultimately bounded to the nominal libration point orbit by applying the Hamiltonian structure-based controller. Numerical simulations demonstrate the performance of the designed control strategy. Halo orbit around the L2 point of the Earth-Moon system is considered as an illustrative example, and various perturbations are taken into account.๋ณธ ๋…ผ๋ฌธ์—์„œ๋Š” ๋ถˆ์•ˆ์ •ํ•œ ๋™์ ํŠน์„ฑ์„ ๊ฐ–๋Š” ๋ผ๊ทธ๋ž‘์ฃผ ์  ๊ถค๋„ ์ฃผ๋ณ€์—์„œ ์œ„์„ฑ์˜ ๊ถค๋„์œ ์ง€ ๋ฐ ํŽธ๋Œ€๋น„ํ–‰์„ ์œ„ํ•œ ์ œ์–ด๊ธฐ์™€ ๊ด€์ธก๊ธฐ๋ฅผ ์„ค๊ณ„ํ•˜์˜€์œผ๋ฉฐ, ์„ค๊ณ„๋œ ์ œ์–ด๊ธฐ์™€ ๊ด€์ธก๊ธฐ์˜ ์•ˆ์ •์„ฑ ๊ทธ๋ฆฌ๊ณ  ์ „์ฒด ์‹œ์Šคํ…œ์˜ ์•ˆ์ •์„ฑ์„ ๋ถ„์„ํ•˜์˜€๋‹ค. ์„ค๊ณ„ํ•œ ๊ธฐ์ค€ ์ œ์–ด ์ „๋žต์€ ์‹ ํ˜ธ์ฒ˜๋ฆฌ ๊ด€์ ์˜ ์ œ์–ด์ด๋ก ์„ ๊ธฐ๋ฐ˜์œผ๋กœ ํ•˜์ง€ ์•Š๊ณ , ๋ผ๊ทธ๋ž‘์ฃผ ์  ๊ถค๋„์˜ ์ž์—ฐ์ ์ธ ์ˆ˜ํ•™์  ๊ตฌ์กฐ๋ฅผ ํ™œ์šฉํ•˜์˜€๋‹ค. ๋ชจ๋ธ ๋ถˆํ™•์‹ค์„ฑ๊ณผ ์™ธ๋ถ€ ์™ธ๋ž€์œผ๋กœ ์ธํ•œ ๊ธฐ์ค€ ์ œ์–ด ์ „๋žต์˜ ์„ฑ๋Šฅ์ €ํ•˜๋ฅผ ์™„ํ™”ํ•˜๊ธฐ ์œ„ํ•ด ์™ธ๋ž€๊ด€์ธก๊ธฐ์˜ ์ผ์ข…์ธ ํ™•์žฅ ๊ณ ์ด๋“ ๊ด€์ธก๊ธฐ๋ฅผ ์„ค๊ณ„ํ•˜์˜€๋‹ค. ๋ณธ ๋…ผ๋ฌธ์—์„œ๋Š” ๊ถค๋„์—ญํ•™์— ๋‚ด์žฌ๋˜์–ด ์žˆ๋Š” ํ•ด๋ฐ€ํ„ด ์‹œ์Šคํ…œ์˜ ๊ตฌ์กฐ๋ฅผ ํ™œ์šฉํ•˜๋Š” ์ œ์–ด๊ธฐ๋ฅผ ์„ค๊ณ„ํ•˜๊ธฐ ์œ„ํ•ด ์ •์ค€์ขŒํ‘œ๋ฅผ ๋„์ž…ํ•˜์˜€์œผ๋ฉฐ, ์ขŒํ‘œ๋ณ€ํ™˜์„ ํ†ตํ•ด ์œ„์„ฑ์˜ ์šด๋™๋ฐฉ์ •์‹์„ ํ•ด๋ฐ€ํ„ด ์‹œ์Šคํ…œ์˜ ์ •์ค€ํ˜•์‹์œผ๋กœ ๋‚˜ํƒ€๋‚ด์—ˆ๋‹ค. ํ•ด๋ฐ€ํ„ด ์‹œ์Šคํ…œ์˜ ์ •์ค€ํ˜•์‹์œผ๋กœ ํ‘œํ˜„๋œ ์šด๋™๋ฐฉ์ •์‹์„ ์ด์šฉํ•ด ์„ค๊ณ„ํ•œ ๊ธฐ์ค€ ์ œ์–ด๊ธฐ๋Š” ํ•ด๋ฐ€ํ„ด-๊ตฌ์กฐ ๋ณด์กด์ œ์–ด์™€ ์—๋„ˆ์ง€ ์†Œ์‚ฐ์ œ์–ด๋กœ ๋ถ„๋ฆฌ ์„ค๊ณ„๋œ๋‹ค. Lagrange-Dirichlet ๊ธฐ์ค€์€ ์ •์ค€ํ˜•์‹์œผ๋กœ ๋‚˜ํƒ€๋‚ธ ํ•ด๋ฐ€ํ„ด ์‹œ์Šคํ…œ์˜ ๋น„์„ ํ˜• ์•ˆ์ •์„ฑ์„ ํŒ๋ณ„ํ•˜๋Š” ์ถฉ๋ถ„์กฐ๊ฑด์œผ๋กœ, ํ•ด๋ฐ€ํ„ด-๊ตฌ์กฐ ๋ณด์กด์ œ์–ด ์„ค๊ณ„์˜ ๊ธฐ์ค€์ด ๋œ๋‹ค. ๊ธฐ์ค€ ๋ผ๊ทธ๋ž‘์ฃผ ์  ๊ถค๋„ ์ฃผ์œ„์—์„œ ํ•ด๋ฐ€ํ„ด-๊ตฌ์กฐ ๋ณด์กด ์ œ์–ด๋ฅผ ์ ์šฉํ•œ ๊ฒฐ๊ณผ, ์œ„์„ฑ์€ ๊ธฐ์ค€๊ถค๋„๋กœ ์ˆ˜๋ ดํ•˜์ง€ ์•Š๊ณ  ๊ธฐ์ค€๊ถค๋„์™€ ์œ ํ•œํ•œ ๊ฑฐ๋ฆฌ๋ฅผ ์œ ์ง€ํ•˜๋Š” ๊ฒฝ๊ณ„์šด๋™์„ ํ•˜์˜€๋‹ค. ๊ฒฝ๊ณ„์šด๋™์˜ ์ฃผํŒŒ์ˆ˜ ๋ถ„์„์„ ํ†ตํ•˜์—ฌ ํŠน์ •ํ•œ ์ดˆ๊ธฐ์กฐ๊ฑด ํ•˜์—์„œ๋Š” ์›ํ˜• ๊ฒฝ๊ณ„์šด๋™์ด ๊ฐ€๋Šฅํ•˜์˜€์œผ๋ฉฐ, ๋” ๋‚˜์•„๊ฐ€ ํ•ด๋ฐ€ํ„ด-๊ตฌ์กฐ ๋ณด์กด์ œ์–ด์˜ ์ œ์–ด์ด๋“ ๊ฐ’์„ ์ ์ ˆํžˆ ์„ค์ •ํ•จ์œผ๋กœ ์›ํ˜• ๊ฒฝ๊ณ„์šด๋™์˜ ํฌ๊ธฐ๋ฅผ ์ฒด๊ณ„์ ์œผ๋กœ ์กฐ์ ˆํ•  ์ˆ˜ ์žˆ๊ณ  ์ด๋ฅผ ์œ„์„ฑ ํŽธ๋Œ€๋น„ํ–‰์— ์‘์šฉํ•  ์ˆ˜ ์žˆ์Œ์„ ๋ณด์˜€๋‹ค. ์ถ”๊ฐ€์ ์œผ๋กœ ์—๋„ˆ์ง€ ์†Œ์‚ฐ์ œ์–ด ์ž…๋ ฅ์„ ์„ค๊ณ„ํ•˜์—ฌ ์œ„์„ฑ์ด ๊ธฐ์ค€ ๋ผ๊ทธ๋ž‘์ฃผ ์  ๊ถค๋„๋กœ ์ ๊ทผ ์ˆ˜๋ ดํ•˜๋Š” ์šด๋™๋„ ๊ฐ€๋Šฅํ•จ์„ ์ˆ˜ํ•™์ ์œผ๋กœ ์ฆ๋ช…ํ•˜์˜€๋‹ค. ํ•œํŽธ, ์‹ฌ์šฐ์ฃผ์ƒ์˜ ์˜ˆ์ธกํ•˜๊ธฐ ์–ด๋ ค์šด ์„ญ๋™๋ ฅ ๋ฐ ๋ถˆํ™•์‹ค์„ฑ ํ•˜์—์„œ๋„ ๊ฐ•๊ฑดํ•œ ๊ถค๋„์œ ์ง€์™€ ํŽธ๋Œ€๋น„ํ–‰์„ ์ˆ˜ํ–‰ํ•˜๊ธฐ ์œ„ํ•ด ํ™•์žฅ ๊ณ ์ด๋“ ๊ด€์ธก๊ธฐ๋ฅผ ์„ค๊ณ„ํ•˜์˜€๋‹ค. ํ™•์žฅ ๊ณ ์ด๋“ ๊ด€์ธก๊ธฐ๋Š” ์œ„์„ฑ์˜ ์œ„์น˜ ์ •๋ณด๋งŒ์„ ์ด์šฉํ•˜์—ฌ ์œ„์„ฑ์˜ ์†๋„์™€ ์œ„์„ฑ์— ์ž‘์šฉํ•˜๋Š” ์™ธ๋ž€์„ ๋™์‹œ์— ์ถ”์ •ํ•˜๋ฉฐ, ์ถ”์ •๋œ ์ƒํƒœ๋ณ€์ˆ˜๋ฅผ ์ด์šฉํ•˜์—ฌ ๊ธฐ์ค€์ด ๋˜๋Š” ํ”ผ๋“œ๋ฐฑ ์ œ์–ด์ž…๋ ฅ์„ ์ƒ์„ฑํ•œ๋‹ค. ์ถ”์ •๋œ ์™ธ๋ž€์€ ํ”ผ๋“œํฌ์›Œ๋“œ ํ˜•ํƒœ์˜ ์ œ์–ด์ž…๋ ฅ์œผ๋กœ ๊ตฌ์„ฑ๋˜์–ด ์ œ์–ด๊ธฐ์˜ ์„ฑ๋Šฅ์„ ๊ฐ•๊ฑดํ•˜๊ฒŒ ๋งŒ๋“ ๋‹ค. ์‹ฌ์šฐ์ฃผ ๊ณต๊ฐ„์ƒ์˜ ์œ„์„ฑ์˜ ๊ถค๋„๊ฒฐ์ • ๊ฒฐ๊ณผ๋กœ ์–ป์–ด์ง€๋Š” ์œ„์น˜์ •๋ณด๋Š” ์ƒ๋Œ€์ ์œผ๋กœ ํฐ ์˜ค์ฐจ๋ฅผ ๊ฐ–๋Š”๋ฐ, ํ™•์žฅ ๊ณ ์ด๋“ ๊ด€์ธก๊ธฐ๋Š” ์œ„์น˜ ์˜ค์ฐจ๋ฅผ ์ฆํญ์‹œํ‚จ๋‹ค๋Š” ๋‹จ์ ์ด ์žˆ๋‹ค. ๋ณธ ์—ฐ๊ตฌ์—์„œ๋Š” ์ด๋Ÿฌํ•œ ๋‹จ์ ์„ ์™„ํ™”ํ•˜๊ณ ์ž ์ ๋ถ„ ๊ด€์ธก๊ธฐ ํ˜•ํƒœ๋กœ ๊ฐœ์„ ๋œ ํ•„ํ„ฐ๋ง๋œ ํ™•์žฅ ๊ณ ์ด๋“ ๊ด€์ธก๊ธฐ๋ฅผ ์„ค๊ณ„ํ•˜๊ณ  ์ˆ˜๋ ด์„ฑ์„ ๋ถ„์„ํ•˜์˜€๋‹ค. ๊ทธ๋ฆฌ๊ณ  ํ•„ํ„ฐ๋ง๋œ ํ™•์žฅ ๊ณ ์ด๋“ ๊ด€์ธก๊ธฐ์™€ ์‹œ์Šคํ…œ์˜ ํ•ด๋ฐ€ํ„ด ๊ตฌ์กฐ๋ฅผ ํ™œ์šฉํ•˜๋Š” ์ œ์–ด๊ธฐ๋ฅผ ์ ์šฉํ•œ ์ „์ฒด ์‹œ์Šคํ…œ์˜ ์•ˆ์ •์„ฑ์„ ๋ถ„์„ํ•˜์˜€๋‹ค. ๋ถˆ์•ˆ์ •ํ•œ ๋ผ๊ทธ๋ž‘์ฃผ ์  ๊ถค๋„ ์ฃผ๋ณ€์—์„œ ์œ„์„ฑ์˜ ๊ถค๋„์œ ์ง€์™€ ํŽธ๋Œ€๋น„ํ–‰์„ ์œ„ํ•ด ์„ค๊ณ„๋œ ์ œ์–ด๊ธฐ๋ฒ•์˜ ์„ฑ๋Šฅ์„ ํ™•์ธํ•˜๊ณ ์ž ์ˆ˜์น˜ ์‹œ๋ฎฌ๋ ˆ์ด์…˜์„ ์ˆ˜ํ–‰ํ•˜์˜€๋‹ค. ์ˆ˜์น˜ ์‹œ๋ฎฌ๋ ˆ์ด์…˜์„ ์œ„ํ•ด ์ง€๊ตฌ-๋‹ฌ ์‹œ์Šคํ…œ์˜ L2 ์ฃผ๋ณ€ ํ—ค์ผ๋กœ ๊ถค๋„๋ฅผ ๊ธฐ์ค€๊ถค๋„๋กœ ์„ค์ •ํ•˜์˜€์œผ๋ฉฐ, ์‹ฌ์šฐ์ฃผ ๊ณต๊ฐ„์—์„œ์˜ ๋‹ค์–‘ํ•œ ์„ญ๋™๋ ฅ ๋ฐ ๋ชจ๋ธ ๋ถˆํ™•์‹ค์„ฑ์„ ๊ณ ๋ คํ•˜์˜€๋‹ค. ๊ถค๋„๊ฒฐ์ • ์˜ค์ฐจ๋กœ ์ธํ•œ ์œ„์„ฑ์˜ ์œ„์น˜ ๋ฐ ์†๋„ ๋ถˆํ™•์‹ค์„ฑ์ด ์กด์žฌ ํ•˜๋”๋ผ๋„ ์ œ์•ˆํ•œ ์ œ์–ด๊ธฐ๋ฒ•์„ ํ†ตํ•ด ์œ„์„ฑ์ด ๊ถค๋„์œ ์ง€์™€ ํŽธ๋Œ€๋น„ํ–‰์„ ๋งŒ์กฑ์Šค๋Ÿฝ๊ฒŒ ์ˆ˜ํ–‰ํ•จ์„ ๋ณด์˜€๋‹ค.1 Introduction 1 1.1 Background and Motivation 1 1.2 Literature Review 3 1.2.1 Spacecraft Station-Keeping in the Vicinity of the Libration Point Orbits 3 1.2.2 Spacecraft Formation Flight in the Vicinity of the Libration Point Orbits 5 1.3 Contributions 7 1.4 Dissertation Outline 10 2 Background 13 2.1 Circular Restricted Three-Body Problem 14 2.1.1 Equilibrium Solutions and Periodic Orbits 16 2.1.2 Stability of Periodic Orbits 20 2.2 Hamiltonian Mechanics 21 2.2.1 Hamiltonian Approach to CR3BP 21 2.2.2 Hamiltonian Approach to LPO Tracking Problem 22 3 Hamiltonian Structure-Based Control 25 3.1 Classical Linear Hamiltonian Structure-Preserving Control 27 3.2 Switching Hamiltonian Structure-Preserving Control 29 3.2.1 Orbital Properties of Spacecraft 33 3.2.2 Switching Point 1: From a Circular Orbit to an Elliptical Orbit 34 3.2.3 Switching Point 2: From an Elliptical Orbit to a Circular Orbit 37 3.3 Hamiltonian Structure-Based Control 39 3.3.1 Potential Shaping Control 39 3.3.2 Energy Dissipation Control 45 4 Filtered Extended High-Gain Observer and Closed-Loop Stability 49 4.1 Filtered Extended High-Gain Observer and Its Convergence 51 4.2 Closed-Loop Stability Analysis 56 5 Numerical Simulations 67 5.1 Disturbance Model 67 5.2 Navigation Error Model 68 5.3 Simulation Results 69 5.3.1 Simulation 1 71 5.3.2 Simulation 2 77 5.3.3 Simulation 3 81 5.3.4 Simulation 4 93 5.3.5 Simulation 5 98 6 Conclusion 101 6.1 Concluding Remarks 101 6.2 Further Work 103 Bibliography 105 ๊ตญ๋ฌธ์ดˆ๋ก 127Docto

    Attitude Control Optimization of a Virtual Telescope for X-ray Observations

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    In this paper, a novel approach is investigated for the attitude control of two satellites acting as a virtual telescope. The Virtual Telescope for X-ray Observations (VTXO) is a mission exploiting two 6U-CubeSats operating in precision formation. The goal of the VTXO project is to develop a space-based, X-ray imaging telescope with high angular resolution precision. In this scheme, one CubeSat carries a diffractive lens and the other one carries an imaging device to support a focal length of 100 m. In this mission, the attitude control algorithms are required to keep the two spacecrafts in alignment with the Crab Nebula observations. To meet this goal, the attitude measurements from the gyros and the star trackers are used in an extended Kalman filter, for a robust hybrid controller. Due to limited energy and the requirement of high accuracy, the energy and accuracy of attitude control is optimized for this mission

    GPS based position control and waypoint navigation of a quad tilt-wing UAV

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    Unmanned aerial vehicles (UAV) are becoming increasingly capable nowadays and the civilian applications and the military tasks that can be carried out by these vehicles are far more critical than before. There have been remarkable advances in the design and development of UAVs. They are equipped with various sensors which make them capable of accomplishing missions in unconstrained environments which are dangerous or effortful for manned aircrafts. Recently, significant interest in unmanned aerial vehicles has directed researchers towards navigation problem of flying vehicles. This thesis work focuses on GPS based position control and waypoint navigation of a quad tilt-wing unmanned aerial vehicle (SUAVI: Sabanci University Unmanned Aerial Vehicle). The vehicle is capable of vertical take-off and landing (VTOL). It can also fly horizontally due to its tilt-wing structure. Mechanical and aerodynamic designs are first outlined. A nonlinear mathematical model expressed in a hybrid frame is then obtained using Newton-Euler formulation which also includes aerodynamics effects such as wind and gusts. Extended Kalman filtering (EKF) using raw IMU measurements is employed to obtain reliable orientation estimates which is crucial for attitude stabilization of the aerial vehicle. A high-level acceleration controller which utilizes GPS data produces roll and pitch references for the low-level attitude controllers for hovering and trajectory tracking of the aerial vehicle. The nonlinear dynamic equations of the vehicle are linearized around nominal operating points in hovering conditions and gravity compensated PID controllers are designed for position and attitude control. Simulations and several real flight experiments demonstrate success of the developed position control algorithms

    1999 Flight Mechanics Symposium

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    This conference publication includes papers and abstracts presented at the Flight Mechanics Symposium held on May 18-20, 1999. Sponsored by the Guidance, Navigation and Control Center of Goddard Space Flight Center, this symposium featured technical papers on a wide range of issues related to orbit-attitude prediction, determination, and control; attitude sensor calibration; attitude determination error analysis; attitude dynamics; and orbit decay and maneuver strategy. Government, industry, and the academic community participated in the preparation and presentation of these papers

    AAS/GSFC 13th International Symposium on Space Flight Dynamics

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    This conference proceedings preprint includes papers and abstracts presented at the 13th International Symposium on Space Flight Dynamics. Cosponsored by American Astronautical Society and the Guidance, Navigation and Control Center of the Goddard Space Flight Center, this symposium featured technical papers on a wide range of issues related to orbit-attitude prediction, determination, and control; attitude sensor calibration; attitude dynamics; and mission design
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