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1978, Astrophysics and Space Science Library
AI
This document provides a comprehensive overview of spacecraft attitude determination, prediction, and control, emphasizing the essential background and ground support aspects necessary for understanding these processes. It serves as a reference for diverse stakeholders, including mission planners, students, and engineers, and is structured to be accessible for those with a foundational knowledge in physics and engineering. The book summarizes critical ideas, data, and techniques while highlighting future activities related to spacecraft attitude support.
Transactions of the Japan Society for Aeronautical and Space Sciences, Space Technology Japan
2005
The work is has been carried from August, 2001 to July, 2005 under the supervision of Assoc. Prof. Thomas Bak. I would like to acknowledge Thomas Bak for his supervision and recommendation of the undersigned for the Ph.D. position. I would also like to thank Prof. Dr. Klaus Briess, Prof. Robert Twiggs, and Assoc. Prof. Rafal Wisniewski for their assessment of the Ph. D. Thesis. A special thanks to Prof. Robert Twiggs for welcoming the undersigned to the Department of Aeronautics and Astronautics, Stanford University, U.S. in 2003 as a visiting researcher, as partial fulfillment of the Ph.D requirements. I would like to acknowledge Dr. Jay Herman at NASA's Goddard Space Flight Center for his assistance with the Earth Probe satellite data product. I would also like to thank Lars Tøffner-Clausen, previously at Danish Meteorological Institute, since moved to the Danish National Space Center, for his assistance in acquiring and post-processing the Ørsted Telemetry Data. Finally I would like to thank Inga Steen-Jensen, my mother, for proof reading the thesis.
2011
The ISS Reshetnev is the Russian leader in development, manufacture and operations of navigation, geodetic and communication spacecraft, as well as Russian State programme for satellite telecommunication systems development. The research results achieved by the ISS Reshetnev in attitude control of some communication spacecraft, are presented.
1996
Planetary penetrator missions offer excellent opportunities for examining the planetary structure in great detail. The success of such missions largely depends on navigating the penetrator to impact the target with the right orientation so that the scientific instruments onboard are safe. This in turn requires a sophisticated autonomous attitude determination and control subsystem (ADCS) onboard the penetrator. The aim of this paper is to propose a suitable mission sequence for such hard landers along with identification of appropriate sensors and actuators, and to examine the attitude determination and control strategies, desired for the right impact. A detailed investigation on using horizon detectors and Sun sensors for attitude determination along with the use of gas jets for attitude control will be discussed. The penetrator is a spin-stabilized platform, and hence a forced precession of the spin axis using the Sun sensor as the reference for firing the thrust pulses results in the penetrator following a rhumb-line attitude trajectory relative to the Sun direction. Results of simulations for the penetrator attitude control targeting the Lunar and Martian surfaces are presented.
AIAA/AAS Astrodynamics Specialist Conference and Exhibit, 2008
was significantly enhanced. The AGSS estimator suite includes a spinning spacecraft Kalman filter and three single-axis attitude estimators: the Fuzzycones method, the Magnetometer-Only Single-Axis Estimator/Calibrator (MOSAEC), as well as a standard differentialcorrector batch-method estimator. The calibration suite of tools includes utilities to estimate relative time offsets, magnetometer calibration parameters, and Sun sensor biases.
Space Science Reviews, 2010
The work presented in this paper concerns the accurate On-Ground Attitude (OGA) reconstruction for the astrometry spacecraft Gaia in the presence of disturbance and of control torques acting on the spacecraft. The reconstruction of the expected environmental torques which influence the spacecraft dynamics will be also investigated. The telemetry data from the spacecraft will include the on-board real-time attitude, which is of order of several arcsec. This raw attitude is the starting point for the further attitude reconstruction. The OGA will use the inputs from the field coordinates of known stars (attitude stars) and also the field coordinate differences of objects on the Sky Mapper (SM) and Astrometric Field (AF) payload instruments to improve this raw attitude. The on-board attitude determination uses a Kalman Filter (KF) to minimize the attitude errors and produce a more accurate attitude estimation than the pure star tracker measurement. Therefore the first approach for the OGA will be an adapted version of KF. Furthermore, we will design a batch least squares algorithm to investigate how to obtain a more accurate OGA estimation. Finally, a comparison between these different attitude determination techniques in terms of accuracy, robustness, speed and memory required will be evaluated in order to choose the best attitude algorithm for the OGA. The expected resulting accuracy for the OGA determination will be on the order of milli-arcsec. Keywords Satellite dynamics 1 Introduction The principal feature of the Gaia astrometry mission is to accurately measure the positions, distances, space motions, and many physical characteristics of about one billion stars in
AIAA Guidance, Navigation, and Control Conference, 2010
Planetary penetrator missions offer excellent opportunities for examining the planetary structure in great detail. The success of such missions largely depends on navigating the penetrator to impact the target with the right orientation so that the scientific instruments onboard are safe. This in turn requires a sophisticated autonomous attitude determination and control subsystem (ADCS) onboard the penetrator. The aim of this paper is to propose a suitable mission sequence for such hard landers along with identification of appropriate sensors and actuators, and to examine the attitude determination and control strategies, desired for the right impact. A detailed investigation on using horizon detectors and Sun sensors for attitude determination along with the use of gas jets for attitude control will be discussed. The penetrator is a spin-stabilized platform, and hence a forced precession of the spin axis using the Sun sensor as the reference for firing the thrust pulses results in the penetrator following a rhumb-line attitude trajectory relative to the Sun direction. Results of simulations for the penetrator attitude control targeting the Lunar and Martian surfaces are presented.
Attitude slew motions for spacecraft are usually undertaken using feedback control where only the desired final attitude is stated. In this paper attitude guidance is considered which could be used, in addition to feedback control, to enhance the efficiency of slew motions by pre-planning time-dependent attitude motions. This is achieved using a three-step method in which the angular velocities are expressed as analytic functions in terms of free parameters (on the virtual time domain), and the boundary conditions on the rotation are matched using a shooting method based on a discretized form of Rodrigue's formula. Following this, the virtual time is reparametrized. This is applied to design a rest-to-rest two-impulse slew manoeuver and a slew motion using only two reaction wheels.
2016
A new spacecraft attitude estimation approach based on the Unscented Filter is derived. For nonlinear systems the Unscented Filter uses a carefully selected set of sample points to more accurately map the probability distribution than the linearization of the standard Extended Kalman Filter, leading to faster convergence from inaccurate initial conditions in attitude estimation problems. The filter formulation is based on standard attitude-vector measurements using a gyro-based model for attitude propagation. The global attitude parameterization is given by a quaternion, while a generalized three-dimensional attitude representation is used to define the local attitude error. A multiplicative quaternion-error approach is derived from the local attitude error, which guarantees that quaternion normalization is maintained in the filter. Simulation results indicate that the Unscented Filter is more robust than the Extended Kalman Filter under realistic initial attitude-error conditions. ...
2004
13 Journal-The Institution of Engineers, Malaysia (Vol. 65, No. 1/2, March/June 2004) thermal management. Consequently, the power budget for these tasks could be suppressed. This article is organized in the following manner: First, the miniaturisation design principle is viewed ...
Journal of Physics: Conference Series, 2013
This work discusses an attitude control study for the ASTER mission, the first Brazilian mission to the deep space. The study is part of a larger scenario that is the development of optimal trajectories to navigate in the 2001 SN263 asteroid system, together with the generation of orbit and attitude controllers for autonomous operation. The spacecraft attitude is defined from the orientation of the body reference system to the Local Vertical Local Horizontal (LVLH) of a circular orbit around the Alpha asteroid. The rotational equations of motion involve the dynamic equations, where the three angular speeds are generated from a set of three reaction wheels and the gravitational torque. The rotational kinematics is represented in the Euler angles format. The controller is developed via the linear quadratic regulator approach with output feedback. It involves the generation of a stability augmentation (SAS) loop and a tracking outer loop, with a compensator of desired structure. It was chosen the feedback of the p, q and r angular speeds in the SAS, one for each reaction wheel. In the outer loop, it was chosen a proportional integral compensator. The parameters are tuned using a numerical minimization that represents a linear quadratic cost, with weightings in the tracking error and controls. Simulations are performed with the nonlinear model. For small angle manoeuvres, the linear results with reaction wheels or thrusters are reasonable, but, for larger manoeuvres, nonlinear control techniques shall be applied, for example, the sliding mode control.
AIAA/AAS Astrodynamics Specialist Conference and Exhibit, 2004
This paper presents the attitude determination method for the Bifocal Relay Mirror Spacecraft Simulator. The simulator simulates three-axis motion of a spacecraft and has an optical system emulating a bifocal space telescope. The simulator consists of three control moment gyroscopes, rate gyros, two-axis analog sun sensor, and two inclinometers. The five-foot diameter platform is supported on a spherical air bearing to offer a low-torque environment. This paper demonstrates two attitude determination methods employing the measurements from a two-axis analog IR sensor, two inclinometers, and a triaxial gyroscope. The first method implements the conventional Kalman filter algorithm. The second method uses a nonlinear observer derived from the Lyapunov's direct method. Analytical and experimental results are presented to validate the proposed algorithm.
2011
Spin-stabilized spacecraft generally rely on sun and three-axis magnetic eld sensor measurements for attitude determination. This study experimentally determines the total accuracy of attitude determination solutions using modest quality sensors. This was accomplished by having a test spacecraft collect data during spinning motions. The data was then post-processed to nd the attitude estimates, which were then compared to the experimentally measured attitude. This same approach will be used to test the accuracy of the attitude determination system of the DICE spacecraft to be built by SDL/USU.
2019
Based on the three-dimensional dynamics of a rigid body and Newton's laws, the simplified dynamics of a spacecraft is studied and described through the systematical representation, mathematical modeling and also by a block diagram representation, to finally simulates the spacecraft dynamics in the Matlab programming environment called Simulink. It is paramount to be able to identify and recognize the attitude (often represented with the Euler angles) and position variables like the degrees of freedom (DOF) of the system and also the linear behavior. All this to conclude up about the non-linear behavior presented by the accelerations, velocities, positions and Euler angles (attitude) when those mentioned are plotted against time. In addition to this, the linearized system is found in order to facilitate the control analysis and stability analysis, at using linear analysis tools of Simulink and concepts like controllability and observability, reaching the point of determining under the previous concepts to proceed with the control design phase. Lastly, an uncertainty and sensitivity analysis is realized, by means the Monte-Carlo and the Linear regression method (in Simulink too), to find the torque like critical model input, since it has the greatest effect on the response variables in the system; and thus finally, to implement the Linear Quadratic Regulator (LQR) controller, at using the lqr Matlab function.
The spacial missions will have a high automati-zation level, making the pointing precision growing up. The control system trust will be very important. It is possible to see that the tests will have more hardware into de software mesh, so the process starts from a control system complete simulation and, slowly, the on board computer and sensors will be added, using the real system parts, and simulating at a computer only what is necessary.
2012
This paper describes a path toward the development of theory for using a low noise high frame rate camera as a star tracker for spacecraft attitude estimation. The benefit of using a low noise high frame rate camera is that s ar data can be sampled at a faster rate while allowing one to measure very di m stars, increasing the number of stars available for attitude estimation. The d evelopment of a noise model is discussed and an algorithm to process raw data is sho wn. An attitude estimation method is discussed and simulated data is shown. A simulated star tracker for attitude estimation is shown and attitude estim ation results are shown.
Advances in Estimation, Navigation, and Spacecraft Control, 2015
Attitude determination, along with attitude control, is critical to functioning of every space mission. In this paper, we investigate and compare, through simulation, the application of two autonomous sequential attitude estimation algorithms, adopted from the literature, for attitude determination using attitude sensors (sun sensor and horizon sensors) and rate-integrating gyros. The two algorithms include a direction cosine matrix (DCM) based steady-state Kalman Filter and the classic quaternion-based Extended Kalman Filter. To make the analysis realistic, as well as to improve the design of the attitude determination algorithms, detailed sensor measurement models are developed. Modifications in the attitude determination algorithms, through estimation of additional states, to account for sensor biases and misalignments have been presented. A modular six degree-of-freedom closed-loop simulation, developed in house, is used to observe and compare the performances of the attitude determination algorithms.
GOES-8 and Beyond, 1996
This paper presents a summary of the basic simulation parameters and results of a study for the Geostationary Operational Environmental Satellite (GOES). The study involves the simulation of minor modifications to the current spacecraft, so that the relative performance of these modifications can be analyzed. The first modification studied requires the placement of a baseline inertial reference unit, such as the Dry Rotor Inertia Reference Unit (DRIRU-II) or the Space Inertial Reference Unit (SIRU), onto the spacecraft. The second modification involves using the imager/sounder assembly for real-time on-board attitude determination information. The third modification studied is the addition of star trackers to provide precise attitude knowledge. Simulation results are presented for each modification.
2003
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Planetary penetrator missions offer excellent opportunities for examining the planetary structure in great detail. The success of such missions largely depends on navigating the penetrator to impact the target with the right orientation so that the scientific instruments onboard are safe. This in turn requires a sophisticated autonomous attitude determination and control subsystem (ADCS) onboard the penetrator. The aim of this paper is to propose a suitable mission sequence for such hard landers along with identification of appropriate sensors and actuators, and to examine the attitude determination and control strategies, desired for the right impact. A detailed investigation on using horizon detectors and Sun sensors for attitude determination along with the use of gas jets for attitude control will be discussed. The penetrator is a spin-stabilized platform, and hence a forced precession of the spin axis using the Sun sensor as the reference for firing the thrust pulses results in the penetrator following a rhumb-line attitude trajectory relative to the Sun direction. Results of simulations for the penetrator attitude control targeting the Lunar and Martian surfaces are presented.
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