Dissertations / Theses on the topic 'Nanosatellites – Control systems'

The objective of this bachelor thesis was to display all the attitude and control systems (ACS) available for CubeSats and how magnetic ACS are the most convenient option in terms of volume. Precisely this project focused on the procedure, the design and the laws of physics that are behind the creation of a torque rod, a magnetic attitude and control system conceived for nanosatellites. After discussing the magnetic laws, the different types of materials of the core, and the geometric parameters of the core and of the wire, all of which determine the operating area of the system, a theoretical model for a torque rod was devised. This was done by using the models present in Niccolò Bellini’s master thesis “Magnetic actuators for nanosatellite attitude control”, 2014. This bachelor thesis ended with the gathering of some experimental data on an embedded magnetorquer collected through a Helmholtz cage.

Thesis (MScEng (Electrical and Electronic Engineering))--University of Stellenbosch, 2009.
The nanosatellite is build-up of subsystems and payloads (defined as satellite nodes) connected together into the OBC using CAN bus as the main communication protocol. The flight software application is required to run within the eCos environment on the OBC to monitor and control satellite nodes. The ground station must generate commands and send them to the satellite in space. The application is developed to validate, schedule and dispatch the commands to the satellite nodes at appropriate times. Each node manager, in the flight software, is required to execute the response messages from its respective satellite node. The housekeeping and error recovery data files are defined to convey useful information about satellite status to the user and can be downloaded to the ground station. The flight software is developed using POSIX functions supported by eCos. Although it is not yet ready for real operation in space, the algorithm that can be used for full development is examined and approved.

CubeSats have become popular among universities, research organizations, and government agencies due to their low cost, small size, and light weight. Their standardized configurations further reduce the development time and ensure more frequent launch opportunities. Early cubesat missions focused on hardware validation and simple communication missions, with little requirement for pointing accuracy. Most of these used magnetic torque rods or coils for attitude stabilization. However, the intrinsic problems associated with magnetic torque systems, such as the lack of three-axis control and low pointing accuracy, make them unsuitable for more advanced missions such as detailed imaging and on-orbit inspection. Three-axis control in a cubesat can be achieved by combining magnetic torque coils with other devices such as thrusters, but the lifetime is limited by the fuel source onboard. To maximize the mission lifetime, a fast attitude control management algorithm that could optimally manage the usage of the magnetic and thruster torques is desirable. Therefore, a recently developed method, the B-Spline-augmented virtual motion camouflage, is presented in this defense to solve the problem. This approach provides results which are very close to those obtained through other popular nonlinear constrained optimal control methods with a significantly reduced computational time. Simulation results are presented to validate the capabilities of the method in this application.
ID: 030646253; System requirements: World Wide Web browser and PDF reader.; Mode of access: World Wide Web.; Thesis (M.S.A.E.)--University of Central Florida, 2011.; Includes bibliographical references (p. 45-49).
M.S.A.E.
Masters
Mechanical and Aerospace Engineering
Engineering and Computer Science
Aerospace Engineering; Space System Design and Engineering Track

Thesis (MEng)-- Stellenbosch University, 2013.
ENGLISH ABSTRACT: The next generation of CubeSats will require accurate attitude knowledge throughout orbit for advanced science payloads and high gain antennas. A star tracker can provide the required performance, but star trackers have traditionally been too large, expensive and power hungry to be included on a CubeSat. The aim of this project is to develop and demonstrate a CubeSat compatible star tracker. Subsystems from two other CubeSat components, CubeSense and CubeComputer, were combined with a sensitive, commercial image sensor and low-light lens to produce one of the smallest star trackers in existence. Algorithms for star detection, matching and attitude determination were investigated and implemented on the embedded system. The resultant star tracker, named CubeStar, can operate fully autonomously, outputting attitude estimates at a rate of 1 Hz. An engineering model was completed and demonstrated an accuracy of better than 0.01 degrees during night sky tests.
AFRIKAANSE OPSOMMING: Die volgende generasie van CubeSats sal akkurate orientasie kennis vereis gedurende 'n volle omwentelling van die aarde. 'n Sterkamera kan die vereiste prestasie verskaf, maar sterkameras is tradisioneel te groot, duur en krag intensief om ingesluit te word aanboord 'n CubeSat. Die doel van hierdie projek is om 'n CubeSat sterkamera te ontwikkel en te demonstreer. Substelsels van twee ander CubeSat komponente, CubeSense en CubeComputer, was gekombineer met 'n sensitiewe kommersiële beeldsensor en 'n lae-lig lens om een van die kleinste sterkameras op die mark te produseer. Algoritmes vir die ster opsporing, identi kasie en orientasie bepaling is ondersoek en geïmplementeer op die ingebedde stelsel. Die gevolglike sterkamera, genaamd CubeStar, kan ten volle outonoom orientasie afskattings lewer teen 'n tempo van 1 Hz. 'n Ingenieursmodel is voltooi en 'n akkuraatheid van beter as 0.01 grade is gedemonstreer.

Thesis (MScEng)--Stellenbosch University, 2011.
ENGLISH ABSTRACT: The Electronic Systems Laboratory at Stellenbosch University is currently developing a fully 3-axis controlled Attitude Determination and Control Subsystem (ADCS) for CubeSats. This thesis describes the design and development of an Onboard Computer (OBC) suitable for ADCS application. A separate dedicated OBC for ADCS purposes allows the main CubeSat OBC to focus only on command and data handling, communication and payload management. This thesis describes, in detail the development process of the OBC. Multiple Microcontroller Unit (MCU) architectures were considered before selecting an ARM Cortex-M3 processor due to its performance, power efficiency and functionality. The hardware was designed to be as robust as possible, because radiation tolerant and redundant components could not be included, due to their high cost and the technical constraints of a CubeSat. The software was developed to improve recovery from lockouts or component failures and to enable the operational modes to be configured in real-time or uploaded from the ground station. Ground tests indicated that the OBC can handle radiation-related problems such as latchups and bit-flips. The peak power consumption is around 500 mW and the orbital average is substantially lower. The proposed OBC is therefore not only sufficient in its intended application as an ADCS OBC, but could also stand in as a backup for the main OBC in case of an emergency.
AFRIKAANSE OPSOMMING: Die Elektroniese Stelsels Laboratorium by die Universiteit van Stellenbosch is tans besig om ’n volkome 3-as gestabiliseerde oriëntasiebepaling en -beheerstelsel (Engels: ADCS) vir ’n CubeSat te ontwikkel. Hierdie tesis beskryf die ontwerp en ontwikkeling van ’n aanboordrekenaar (Engels: OBC) wat gebruik kan word in ’n ADCS. ’n Afsonderlike OBC wat aan die ADCS toegewy is, stel die hoof-OBC in staat om te fokus op beheer- en datahantering, kommunikasie en loonvragbestuur. Hierdie tesis beskryf breedvoerig die werkswyse waarvolgens die OBC ontwikkel is. Verskeie mikroverwerkers is as moontlike kandidate ondersoek voor daar op ’n ARM Cortex-M3-gebaseerde mikroverwerker besluit is. Hierdie mikroverwerker is gekies vanweë sy spoed, effektiewe kragverbruik en funksionaliteit. Die hardeware is ontwikkel om so robuust moontlik te wees, omdat stralingbestande en oortollige komponente weens kostebeperkings, asook tegniese beperkings van ’n CubeSat, nie ingesluit kon word nie. Die programmatuur is ontwikkel om van ’n uitsluiting en ’n komponentfout te kan herstel. Verder kan programme wat tydens vlug in werking is, verstel word en vanaf ’n grondstasie gelaai word. Grondtoetse het aangedui dat die OBC stralingverwante probleme, soos ’n vergrendeling (latchup) of bis-omkering (bit-flip), kan hanteer. Die maksimum kragverbruik is ongeveer 500 mW en die gemiddelde wentelbaankragverbruik is beduidend kleiner. Die voorgestelde OBC is dus voldoende as ADCS OBC asook hoof-OBC in geval van nood.

Thesis (MEng) Stellenbosch University, 2014
ENGLISH ABSTRACT: An Attitude Determination and Control System (ADCS) demonstrator and testing platform was required for satellite engineering students. The ADCS demonstrator and testing platform will allow students to develop insight into the concepts and challenges of ADCS design and implementation. The existing model nano-satellite EyasSAT was used as a design platform for a new ADCS demonstrator. A new ADCS module (ADCS_V2) was developed to replace the existing EyasSAT ADCS module. The new module allows for three-axis ADCS and the demonstration of the ADCS on an air bearing platform. The air bearing allows full freedom of movement for yaw rotations with limited pitch and roll rotations. The actuators and sensors required for the ADCS were developed and integrated into EyasSAT. In addition a new PCB was designed to form the ADCS_V2 module. Attitude determination algorithms and attitude control algorithms were implemented and tested using MATLAB Simulink simulations. These algorithms were then implemented on the ADCS_V2 module. The ADCS was tested using Hardware In the Loop (HIL) techniques and an air bearing. The yaw attitude of EyasSAT could be controlled within 0.4 degrees accuracy with all the sensors active. In order to stabilize the air bearing platform, the pitch and roll angles were rate controlled. The pitch and roll rates were damped to within 6 mrad/s.
AFRIKAANSE OPSOMMING: ’n Oriëntasiebepaling en Beheerstelsel (OBBS) demonstrasie en toets platform was benodig vir satellietingenieurswese studente. Die nuwe OBBS sal studente toelaat om insig te ontwikkel met betreking tot die idees en uitdagings wat verband hou met die ontwikkeling en implementering van ’n OBBS. Die huidige nano-sateliet model EyasSAT was gebruik as ’n ontwerpsbasis vir die nuwe OBBS. Die nuwe OBBS was ontwikkel om die huidige module van EyasSAT te vervang. Die nuwe OBBS laat oriëntasiebepaling en -beheer in drie asse toe. Die nuwe OBBS en EyasSAT kan die werking van ’n OBBS demonstreer op ’n luglaerplatform. Die luglaer laat vrye rotasie om die gierhoek toe terwyl die rol- en stygings-as beperk word. Die aktueerders en sensors wat benodig word vir die OBBS is ontwikkel en geïntegreer in EyasSAT saam met ’n nuwe gedrukte stroombaanbord om die nuwe OBBS te vorm. Orientasiebepaling en orientasiebeheer algoritmes is geïmplementeer en getoets met die hulp van MATLAB Simulink simulasies. Die algoritmes was op die OBBS module geïmplementeer en getoets deur gebruik te maak van HIL tegnieke en praktiese toetse op die luglaer. Die rotasie hoek van EyasSAT kan met ’n akkuraatheid van 0.4 grade beheer word indien al die sensors gebruik word. Die rol en stygingshoeksnelheid was gekanselleer om die luglaer stabiel te hou. Die hoeksnelheid van die twee asse kon tot kleiner as 6 mrad/s beheer word.

Thesis (MTech(Electrical Engineering))--Cape Peninsula University of Technology, 2011.
Nanosatellite is an electronic device that requires a steady and reliable electrical power supplier (EPS) in order to drive all its electronic circuits. Its unpredictable failures can lead to extensive financial and time losses. The failures may be owing to the environment in which the satellite operates; the technique and the method used to generate power. In order to effectively minimise the risk of the EPS failures, a better technique is essential. The direct energy transfer (DET) technique was chosen for this research because it provides high efficiency and high reliability, unlike the maximum power point tracking (MPPT) technique, which obtains maximum power from the solar cells by using a microcontroller. DET works on a fixed working point of current-voltage characteristic and responds to all satellite power system requirements. The microcontroller is not a suitable device in satellite electrical power systems that requires high reliability, but is used because it is difficult to track the maximum power of solar cells without it. The analog MPPT system is another option, but the technique requires discrete components. Its deployment is limited because of the system's operating frequency and large electronic components such as the inductor and capacitor.

Depuis les tous premiers jours de l'ère spatiale, les satellites artificiels ont été considérés comme un outil pour la résolution de problèmes scientifiques et pratiques, notamment dans l'astronomie, l'observation de la Terre et les télécommunications. Traditionnellement, les gros satellites artificiels, avec une masse allant de plusieurs centaines de kilogrammes jusqu'à plusieurs tonnes, ont été utilisés pour ces besoins. Un élément clef pour permettre le succès de ces missions spatiales est un contrôle précis de l'attitude du satellite. Afin d'assurer la haute précision de pointage, un système de contrôle d'attitude et d'orbite (SCAO) repose sur les données fournies par un instrument optoélectronique appelé un senseur stellaire (ou Star Tracker, ST). L'utilisation des étoiles éloignées comme points de repère permet la détermination de l'attitude du satellite avec une précision de l'ordre de la seconde d'arc. Beaucoup de travaux sur la miniaturisation des sous-systèmes des satellites artificiels ont été entrepris au court des vingt dernières années. Cela a permis à l'industrie et aux passionnés de développer et construire des satellites de quelques kilogrammes pouvant accomplir de véritables missions spatiales. Centaines de ces satellites appelés « nano-satellites » sont lancé chaque année et certains parmi eux peut être considéré comme un replacement des gros satellites. Cependant, dû à de grosses contraintes de masse et de volume définis par les standards na no-satellites, tel que lU-3U CubeSat Design Specification, l'intégration de senseur stellaire dans ces nano-satellites n'était jusqu'à présent pas possible, limitant l'application de ces plateformes. Dans ce travail, senseur stellaire est considéré comme un système composé par un module caméra et un module de traitement d'image. les solutions possibles pour chaque module sont analysées séparément dans un contexte de miniaturisation de ST par modélisation et simulation. Elles sont ensuite évaluées ensemble comme les prototypes fonctionnels dans un installation hardware-in-the-loop (Hll). Cette recherche aborde plusieurs problèmes liés à la miniaturisation d'optique de caméra et du capteur d'image à pixel actif (active pixel sensor, APS), tels que la sensibilité réduite à la lumière des étoiles et l'incertitude de position des centroïdes à cause de la distorsions et l'aberrations chromatique d'optique miniaturisée. L'évaluation dans l'installation Hll se concentre autour des performances du module de traitement et plus particulièrement sur les performances du logiciel ST dans le mode d'opération « perdu dans l'espace» ("Iost-in-space", LIS). Une contribution originale de cette recherche est un algorithme de reconnaissance d'étoiles (StarID) nommé « RING-O » développé et breveté par l'auteur. Par rapport aux autres algorithmes existants, RING-O peut facilement être adapté et ajusté à différentes caméras et plateformes de traitement. Des implémentations logicielles d'algorithme ont été effectuées sur deux prototypes, l'un basé sur smartphone et l'autre basé sur une plateforme Xilinx Zynq, afin de réaliser une analyse des goulets et d'extraire les performances du système. Optimisé pour les plateformes multi-coeurs, RING-O garantit les délais d'acquisition initiale d'attitude comparable et souvent plus petits que les délais d'acquisition déclaré par les autres développeurs de senseur stellaires européens
From the early days of the space age, satellites were considered as a solution for many scientific and practical tasks, notably astronomy, Earth observation and telecommunication. Traditionally and to the present day, mostly large satellites with a mass from several hundred kilograms to several tons are used for these purposes. The key success factor of such space missions is a fine control of satellite’s attitude. To ensure high pointing accuracy, satellite’s attitude determination and control subsystem (ADCS) relies on precise three-dimensional attitude data provided by an opto-electronic instrument called star tracker (ST). The use of stars as reference objects allows to determine the satellite’s attitude in real time with an arc-second precision.A significant work on miniaturization of satellite subsystems carried out in the past twenty years, allows us today to build a complete satellite with a mass of only a few kilograms. An increasing number of successful nano- and picosatellite missions demonstrates constantly improving capabilities of modern miniaturized satellite platforms. However, until recently, integration of a star tracker into a nanosatellite was not possible because of a large size of the device and relatively high power consumption, and that limited possible applications of the nanosatellites. In attempt to change the situation, in the last five years about a dozen of miniature star tracker prototypes, suitable for nanosatellite platforms, were proposed by various developers. Some were successfully tested in space, yet most prototypes, including the tiniest ones, are still at the development stage.A modern star tracker is a system, that can be represented as two modules, a digital camera module and a processing module. Use of a compact camera lens and a small-size image sensor allows to significantly reduce overall mass and size of the device, and at the same time, may cause significant image quality deterioration, due to increased distortion, uncompensated spherical and chromatic aberration, lower signal-to-noise ratio (SNR) and overall lower light sensitivity of the camera module. Thus, embedded software of the processing module, responsible for pre-processing, star identification and attitude calculation, should take into account the limitations imposed by the miniaturization of the camera module. At the same time, hardware architecture of the processing module should have the capacity to perform necessary correction of the digital image in real time, and to ensure stability and expected performance of the star identification and attitude calculation routines.The goal of hardware and software prototyping of a miniature star tracker system, carried out in this work, is to evaluate various design solutions, that could be brought into the camera or into the processing module, in order to help the miniaturization of the system. Another goal is to analyze the impact of every hardware and software component on the overall performance of a miniaturized star tracker system. Among the list of star tracker characteristics, the initial attitude estimation time and the attitude output rate became the focus of the research. Current work addresses possible performance bottlenecks, that may appear on any step of star tracker operation, from capturing starlight to calculation of components of the attitude quaternion, and proposes an original solution to speed-up the star identification routine

Thesis (M.S. in Mechanical Engineering)--Naval Postgraduate School, December 2009.
Thesis Advisor(s): Romano, Marcello ; Bevilacqua, Riccardo. "December 2009." Description based on title screen as viewed on January 27, 2010. Author(s) subject terms: spacecraft, cubesat, nanosat, TINYSCOPE, simulator, test bed, control, system identification, least squares, adaptive mass balancing, mass balancing, three axis simulator, NACL, TAS, CubeTAS, ADCS. Includes bibliographical references (p. 77-82). Also available in print.

M. Tech. Electrical Engineering
The topic of this dissertation is the attitude control of a CubeSat in an elliptic orbit using nonlinear control. The attitude control system (ACS) is a subsystem of a CubeSat. Its principal goal is to stabilise the orientation of the satellite after launch and during the orbital motion of the satellite. Although several methods have been applied to achieve this objective, this still remains a challenging objective and hence plays an integral role in many modern technologies. CubeSat "Cube Satellite" is a miniaturised satellite which, due to its low cost and application potential is often used by academic institutions for research purposes. However, due to its physical size and weight of 1 kilogram, CubeSat have comparatively limited power supply and computational resources; hence the need for an uncomplicated and reliable control system is critical.

M. Tech. Electrical Engineering
Deals with nonlinear methods for magnetic attitude control and reaction wheel attitude control. The work is divided into a number of parts. The first part, deals with the satellite attitude control basic information and development of a mathematical model of a low Earth orbit satellite. The second part introduces the controllers used in this dissertation. The third part deals with the dimension between the output of controller and input of reaction wheel. The fourth part solves the problem of the magnetic torque calculation. The last part carries out the simulation tests of those controllers for small satellite and cube satellite.

碩士
國立成功大學
航空太空工程學系碩博士班
101
The thesis describes the implementation of an active attitude determination and control system (ADCS) for the PACE nanosatellite. PACE satellite is a 2U cubesat under developed at National Cheng Kung University (NCKU) with a mass less than 2 kg and dimension of 100 mm x 100 mm x 227 mm. Two main missions of PACE satellite are to conduct attitude control experiments and to demonstrate the technology to be used in future missions for small satellite. The ADCS sub-system aims to provide functions for active attitude control such as detumbling, determination and stabilization. More importantly, the operation of the PACE mission will allow users to upload ADCS algorithms so that the algorithm can be tested and verified in space. In order to fully verify the embedded ADCS software, a verification system and a Processor-in-the-loop (PIL) simulation are developed. The simulation models consisting of space environment, orbit dynamic, attitude dynamic, and sensor/actuator are modeled using Labview software. A CompactRIO real-time controller is adopted as a simulator to execute simulation models into Labview and also to provide real-time interface with ADCS board. For the results, algorithms and functions for ADCS software are both implemented and verified. The results are met the requirements for ADCS.

The Generic Nanosatellite Bus (GNB) is a spacecraft platform designed to accommodate the integration of diverse payloads in a common housing of supporting components. The development of the GNB at the Space Flight Laboratory (SFL) under the Canadian Advanced Nanospace eXperiment (CanX) program provides accelerated access to space while reducing non-recurring engineering (NRE) costs. The work presented herein details the development of the attitude determination and control subsystem (ADCS) of the GNB. Specific work on magnetorquer coil assembly, integration, and testing (AIT) and reaction wheel testing is included. The embedded software development and unit-level testing of the GNB sun sensors are discussed. The characterization of the AeroAstro star tracker is also a major focus, with procedures and results presented here. Hardware models were developed and incorporated into SFL's in-house high-fidelity attitude dynamics and control simulation environment. This work focuses on specific contributions to the CanX-3, CanX-4&5, and AISSat-1 nanosatellite missions.