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Dissertations |
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WILLIAM HUMBERTO ÚSUGA GIRALDO
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Mask technique for detecting space debris with ground telescope images acquired in static mode
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Advisor : JOSE DIAS DO NASCIMENTO JUNIOR
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COMMITTEE MEMBERS :
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JOSE DIAS DO NASCIMENTO JUNIOR
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JEFFERSON SOARES DA COSTA
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LEANDRO DE ALMEIDA
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Data: Jan 31, 2022
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Show Abstract
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Orbital debris of approximately 10 cm in size can be measured with ground-based telescopes. This debris threatens the functioning of satellites and has an impact on the economy and the global security of space activities. In the GEO orbit, where most of the economically active satellites are located, exists approximately 842 cataloged debris. On the other side, orbiting LEO exists approximately 13485 debris cataloged. In this context, the ESA studies show that hundreds of millions of small objects over 1 mm are currently in the two orbits GEO and LEO above the Earth and have not yet been cataloged. In this study, we created a computational procedure to detect space debris in GEO orbit based on images obtained from ground-based telescopes on the static mode. In this mode, the field sky stars appear as lines in the CCD images and the garbage in the form of dots. CCD images of 2992 x 2092 pixels (high resolution) and with 5 degrees of field of view (FOV) and with 7 seconds of exposure used in this work were obtained with the PanEOS telescope (Panoramic Electro-Optical System), 750 mm aperture, and installed at the Picos dos Dias observatory of the National Astrophysics Laboratory (LNA). For this research, we adapted the Photoutils package written in Python to build a mask and separate stars from candidates for space debris. Our methodology consisted of first smoothing the images using a Gaussian Kernel filter, then each element was categorized into two categories, and finally, the stars were erased resulting only in space debris candidates. We tested combinations of flow to establish the detection limit and used the different points spread function (PSF) to determine the limit of the elongation of objects. Our methodology works with a single image at a time in a fast and efficient way. This allows us to detect objects with different PSF and therefore requires low hardware capability. Our results in this validation phase identified 100% of the artificial training debris. In the real images of the PanEOS telescope, we detected a few real debris consistent with the expected size. In the next steps, we must estimate the size of the object and characterize its orbit.
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2
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JULIANA JENIFFER FERNANDES DE SOUZA RÊGO
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Ballistic armor design of the as-350 helicopter from numerical-experimental analyses.
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Advisor : DINO LINCOLN FIGUEIROA SANTOS
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COMMITTEE MEMBERS :
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DINO LINCOLN FIGUEIROA SANTOS
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JOSE DANIEL DINIZ MELO
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JOSÉ VIRGÍLIO GUEDES DE AVELLAR
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VIVIANE MUNIZ FONSECA
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Data: Feb 14, 2022
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Show Abstract
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Helicopters used in public safety operations go through several risk situations involving ballistic projectiles, one of the safest solutions is armor, offering maximum protection combined with technology.
The present work aims to project an armoring system for the AS-350 helicopter, using as material the polymer matrix composite reinforced with para-aramid fiber and glass fiber. Considering the airworthiness requirements and the restrictions determined by the manufacturer, an analytical method was used to study the effects of armor on the weight and balance of the aircraft. The project used the Aerospace Design Methodology in conducting the work.
To verify the efficiency of the ballistic composite, the experimental tests were carried out in an open outdoor environment where the composite was exposed to the impact of projectiles with a caliber of 5.56x45 mm. The performance of the material was analyzed by the results obtained in the tests and, this provided the determination of the protection reliability of the ballistic system.
The armor design for the AS-350 proved to be safe to be installed on aircraft of this model, as a level III ballistic protection tool, without impairing its mobility.
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3
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ELDER SAMUEL TAVEIRA DA SILVA
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PRELIMINARY DESIGN OF A NANOSATELLITE LAUNCH VEHICLE USING SCRAMJET TECHNOLOGY
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Advisor : DOUGLAS DO NASCIMENTO SILVA
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COMMITTEE MEMBERS :
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DOUGLAS DO NASCIMENTO SILVA
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JOSE HENRIQUE FERNANDEZ
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PAULO GILBERTO DE PAULA TORO
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JOÃO FELIPE DE ARAÚJO MARTOS
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Data: Feb 17, 2022
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Show Abstract
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This Master's Dissertation presents a preliminary design of an aerospace vehicle, using hypersonic airbreathing propulsion based on supersonic combustion (scramjet technology), for atmospheric flight at 20 km altitude, at hypersonic speed, corresponding to Mach number 5.79. Scramjet is an aeronautical engine without moving parts, where the aerospace vehicle integrated with scramjet technology (propulsion system) must be coupled to a rocket engine. The current means of access to space is limited by the chemical propulsion system (solid and / or liquid fuel) carried onboard rockets. The technology of supersonic combustion (scramjet) is being studied as an airbreathing propulsion system, to be used in the dense layers of the Earth's atmosphere, to access space. A demonstrator is being designed to be coupled to the Sonda III rocket engine, to operate as a second stage, starting the operation at 20 km altitude. The theory of oblique shock waves, the theory of heat addition in one-dimensional flow (Rayleigh's theory) and the theory of expansion waves (by Prandtl-Meyer) coupled to the area ratio are applied in the design of the compression sections, of combustion and expansion, respectively, of the scramjet demonstrator with internal admission configuration. Steady state, one-dimensional flow and air under calorically perfect gas conditions will be considered. Thermodynamic properties (pressure, temperature, density, speed of sound) and flow velocity (Mach number) will be presented along the streamline from the leading edge to the trailing edge of the demonstrator, considering flow without and with boundary layer effects, for the conditions of no fuel burning (power-off) and fuel burning (power-on). Finally, the conceptual design and a brief approach to systems engineering in the development of a nanosatellite launch vehicle are presented.
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4
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MARCOS VINICIUS SABINO PEREIRA
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Preliminary design of a scramjet to insert cubesat into orbit
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Advisor : SANDI ITAMAR SCHAFER DE SOUZA
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COMMITTEE MEMBERS :
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DOUGLAS DO NASCIMENTO SILVA
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HEIDI KORZENOWSKI
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PAULO GILBERTO DE PAULA TORO
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SANDI ITAMAR SCHAFER DE SOUZA
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Data: Feb 19, 2022
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Show Abstract
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In order to access the space through the application of hypersonic airbreathing propulsion technology, this work proposes the development of a scramjet (supersonic combustion ramjet). The aerospace vehicle proposed in this work will have three stages, two stages of rocket engines with solid propulsion and a stage composed by a scramjet with four combustion chambers. The scramjet of this vehicle will operate in vertical flight in the Earth’s atmosphere, from 20 km to 60 km of altitude with hypersonic speed corresponding to approximately Mach number 5.8. Bearing in mind that the scramjet has no moving parts and needs a system that accelerates it, up to supersonic combustion conditions, it will be necessary to use the accelerator vehicle that is responsible for propelling the scramjet to the ideal operating conditions (Mach number, position, dynamic pressure). This aerospace vehicle will have the utility of accessing space and conducting drilling experiments, injecting CubeSat into orbit and training the specialized labor responsible for aerospace operations. For the preliminary development of this work, it is necessary to use the theories referring to the formation of shock waves and expansion waves, in addition to the theories related to the addition of heat and the formation of a boundary layer in flow with hypersonic velocity. Therefore, for this development the analytical theoretical methodology was applied and then with the results obtained it was possible to carry out, in the near future, the preliminary mechanical design that determines the necessary basic measures, in addition to the possible materials to be used in the vehicle. The preliminary results of this work indicate that the scramjet will be able to generate thrust and that when considering the existence of the boundary layer, a change in the geometry of the vehicle's inlet is necessary, so that it is possible to maintain the formation of shock-on-lip and shock-on -corner in the scramjet structure.
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5
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ARTHUR BANDEIRA LUZ DE LIMA
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A study about the influence of the solar cycles in the atmospheric conditions over the Curitiba Flight Information Region
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Advisor : JOSE HENRIQUE FERNANDEZ
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COMMITTEE MEMBERS :
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DINO LINCOLN FIGUEIROA SANTOS
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FILIPE EMANUEL VIEIRA TAVEIROS
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JOSE HENRIQUE FERNANDEZ
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Data: Feb 21, 2022
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Show Abstract
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Atmospheric conditions are mostly driven by the Sun, which follows a cycle of activity whose duration is about 11 years. Since this cycle has been found out, researchers has brought up the hypothesis that it may have some influence at the lower atmosphere, taking as proxies the Carbon-14 and Berilium-10 concentration in tree rings and ice cores. Beside that, some manuscripts have shown that, during the Maunder Minimum, where the Sun were at minimum of activity, some regions over the globe experienced a tiny "Ice Age". Initially, it was believed that this influence was related to the Total Solar Irradiation variation during a cycle. Although, further studies have shown that such variations were a rather small to produce these variations on the lower atmosphere. So, they have created the hypothesis that these influence was related to the solar cycle on the Galactic Cosmic Rays (GCR) flux through the heliosphere. GCR work as a ionizing agent, favoring the aerosol synthesis, which acts as Condensation Nuclei, which favors clouds formation. So, the objective of the research was to find a correlation between the solar cycles and meteorological conditions in the region where the cities of Rio de Janeiro e São Paulo are located. In this region, a huge flux of aircraft is observed.
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6
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BENJAMIM MONTEIRO DA SILVA NETO
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DEVELOPMENT A MOBILE PLATAFORM APP FOR THE RISK MANAGEMENT OF NANOSATELLITE PROJECTS
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Advisor : GIULIANI PAULINELI GARBI
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COMMITTEE MEMBERS :
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FRANCISCO JOSÉ TARGINO VIDAL
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GIULIANI PAULINELI GARBI
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MARCOS AURELIO FERREIRA DOS SANTOS
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Data: Feb 22, 2022
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Show Abstract
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Within Systems Engineering, risk management processes are mandatory requirements in satellite missions, being used on a large scale for large satellites. However, traditional approaches need adaptations to be applied, in a viable way, to missions with small satellites due to the costs and deadlines involved. This work aims to design, implement, and disseminate a risk management methodology adapted to small satellites. To this end, it is proposed to create an application to perform this management, using the necessary adaptations for application to this type of mission. The bibliographic research methodology was used to characterize small satellites, mostly the CubeSat platform, and the description of methods and risk management tools used worldwide, as well as their applications to small satellite projects. For the design of the application, the Java language will be used. The application’s functionalities were chosen to provide agility, ease, and integration with the risk management processes. The work is divided into five chapters. The first one consists of an introduction. The second presents a historical reinterpretation of small satellites, definitions of them, and their importance. The third chapter deals with systems engineering and risk management. The fourth chapter presents examples of risk management adapted for nanosatellites. And the fifth chapter presents the proposed solution to the problem raised.
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7
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RAFAEL ALVES FREIRE
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Stellar Rotation Period Versus Energy Variation of Flares in TESS Stars of Spectral Types K and M
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Advisor : JOSE HENRIQUE FERNANDEZ
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COMMITTEE MEMBERS :
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JOSE HENRIQUE FERNANDEZ
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DOUGLAS DO NASCIMENTO SILVA
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JOSE RENAN DE MEDEIROS
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ANTONIO CARLOS DA SILVA MIRANDA
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Data: Feb 24, 2022
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Show Abstract
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Under the development of new technologies, the Aerospace Engineering is increasingly improving its equipments in order to assist exploration that goes beyond our Heliopause. As an example of this we can cite the launch of the space artfact Transiting Exoplanet Survey Satellite (TESS) that has been contributing photometric data to Space Sciences, like Astrophysics, with the aim of study various physical phenomena. As an exemple, the magnetic activity of stars can be fundamental in forming the atmosphere of exoplanets and impact your habitability as well as, it can trigger life in the orbit of type K and M stars, which are considered to be cold and they are the most numerous in the main sequence phase in the Hertzsprung-Russell diagram. Based on these investigations and through statistical analysis of the behavior of stellar flares in relation to their classi cations, rotational periods and spectral subtype, this dissertation presents a study on the variation of energie of stellar flares as a function of their rotational period in a sample of 679 TESS stars of spectral type K and M. None of the stars in this sample showed a correlation between the energy of their surface stellar eruptions as a function of their rotational period. Finally we present four scenarios involving the stars and their stellar eruptions and theirs that can explain our results.
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8
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THIAGO FONSECA MESSIAS
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Test of a UHF receiver to collect satellite sensor data
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Advisor : JOSÉ MARCELO LIMA DUARTE
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COMMITTEE MEMBERS :
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FRANCISCO DE ASSIS BRITO FILHO
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FRANCISCO JOSÉ TARGINO VIDAL
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JOSÉ MARCELO LIMA DUARTE
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Data: Feb 25, 2022
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Show Abstract
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This master’s thesis presents a test plan, the automation system for carrying out the experiments and the results obtained from the Environmental Data Collector (EDC), UHF receiver for collecting data from satellite sensors. The parameters tested were: bandwidth, linearity, spurious, noise figure and performance of the decoding the received signals. The EDC will act in the space segment of the Brazilian Environmental Data Collection System (SBCDA), a forwarding system for satellite message. For over twenty years, the SBCDA has provided data for various surveys. sas, however, the SBDCA needs an update to its space segment. The Institute National Space Research Institute is developing a constellation of nanosatellites from the CubeSat standard to replace the current SBCDA satellites. The EDC will be the payload of the new SBCDA nanosatellites. To validate the EDC, a test plan was prepared which aims to assess whether the prototype built is in accordance with the desired specifications. To carry out the tests, a bench equipped with a computer was built, equipped with testing software, a signal generator, a voltage source and a Arduino. A spectral analysis, from the digitized signal, was used for the tests. of the RF-Front-End and the Frame Error Rate calculation was used to validate the capacity of the EDC to decode incoming messages. The EDC prototype was approved with based on the results obtained, however, some corrections were suggested.
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9
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JOÃO BATISTA DOLVIM DANTAS
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Antennas for the Long Distance Communication System for Unmanned Air Vehicle
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Advisor : FRANCISCO JOSÉ TARGINO VIDAL
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COMMITTEE MEMBERS :
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FILIPE EMANUEL VIEIRA TAVEIROS
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FRANCISCO JOSÉ TARGINO VIDAL
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GIULIANI PAULINELI GARBI
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JOSE PATROCINIO DA SILVA
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Data: Aug 29, 2022
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Show Abstract
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Brazilian Space Launch Centers employ conventional aircraft to monitor large maritime areas destined to the impact point of rockets or parts of them, and this has a high cost. The remotely piloted aircraft (RPAs) have shown to be a low cost solution for operations of this type, however, the short range of their conventional remote controls is a limiting factor for their employment in large distances. This paper proposes high-performance antennas for remotely piloted aircrafts (RPA) communication system, aiming control and image transmission from RPA operating at long distances. It was considered the case-study of the Brazilian Space Launch Centers, which plan to employ RPA in order to assist the surveillance of the restricted area for rocket impact. The proposed antennas were designed in order to maximize gain and lobe aperture for the ground station operation; whereas, for RPA operation, the antennas were tailored in order to provide optimal gain and omnidirectional transmission, even during RPA maneuvers, as well as to minimize weight, size and aerodynamic drag in the aircraft. It is minutely described the design and evaluation of the proposed antennas, by means of simulations and experimental verification. The radio link using the proposed antennas was evaluated in laboratory and verified able to perform data transmission at emulated distance of 110 km (59.4 NM)(68.35 M).
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10
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PAULO CÉSAR DE OLIVEIRA JÚNIOR
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Conception, design and structural analysis of a supersonic combustion demonstrator
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Advisor : JOÃO CARLOS ARANTES COSTA JÚNIOR
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COMMITTEE MEMBERS :
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CREUZA
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HEIDI KORZENOWSKI
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JOÃO CARLOS ARANTES COSTA JÚNIOR
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PAULO GILBERTO DE PAULA TORO
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Data: Dec 14, 2022
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Show Abstract
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ABSTRACT
In the current scenario of the aerospace sector, there is a great limitation related to the payload that can be launched into orbit or beyond. Rocket engines, propulsive technology in operation, have a low specific impulse compared to systems with airbreathing propulsion (scramjet technology) that use atmospheric air as an oxidant. During hypersonic flight, aerospace vehicles with hypersonic airbreathing propulsion are subject to high aerodynamic and thermal loads. In this context, in the present work the main objective is to perform a structural analysis of a generic supersonic combustion demonstrator, under flight conditions at an altitude of 23 km and speed corresponding to Mach 5,8. To carry out the structural analysis, an aerodynamic and dimensional design of a generic scramjet was carried out, designed for coupling to the national rocket engines S30 and S31. Optimization criteria were applied to the compression section, aiming to achieve the required temperature and Mach number conditions at the entrance of the combustion chamber to spontaneously burn hydrogen. In the expansion section, the optimization criterion is based on checking the point at which the pressure condition is equivalent to that of free flow, defining the region where the coupling to the accelerator vehicle must be carried out. The aerodynamic load was defined from analytical and numerical aerodynamic analysis, considering air as a calorically perfect gas and neglecting viscous effects. The design and aerodynamic analysis evaluated the case without fuel burning (power-off) and with fuel burning (power-on), but in the structural analysis only power-on was considered. Numerical flow analysis and numerical structural analysis were respectively performed in the Fluent and Static Structural modules of the Ansys software. The aerodynamic analysis showed that flying at an altitude of 23 km with a speed of 1723 m/s, the scramjet with three compression ramps with deflection angles of 7,48°, 8,93° and 10,77° is capable of generating, at the entrance to the combustion chamber, speed corresponding to Mach number 1,709 and static temperature of 1071,255 K, demonstrating the possibility of burning hydrogen. At the trailing edge, the flow velocity is 1688,958 m/s without fuel burning and 1806,977 m/s with fuel burning, demonstrating that the scramjet is only capable of generating thrust with fuel ignition. For the numerical analysis of the flow, the unstructured mesh with triangular elements proved to be more suitable to capture the flow conditions after the oblique shock waves in the scramjet, considering atmospheric air as a calorically perfect gas and without viscous effects. In the aerodynamic analysis the numerical results showed good agreement with the analytical results. In the numerical structural analysis, the maximum von-Mises equivalent stress is 122,93 MPa and occurs at the leading edge of the fairing, close to contact with the side panel, due to the thickness of the wedge at the leading edge and the high pressures of the chamber of combustion. However, this value is lower than the yield stress of the materials used, so that strains and displacements in the structure occur in the elastic regime of the materials and are therefore recoverable.
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11
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WILLIAM HENRIQUE DE LIMA FIUZA
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Conception, Design and Structural Analysis of an Academic Shock Tube
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Advisor : PAULO GILBERTO DE PAULA TORO
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COMMITTEE MEMBERS :
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DOUGLAS DO NASCIMENTO SILVA
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CREUZA
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PAULO CELSO GRECO JÚNIOR
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PAULO GILBERTO DE PAULA TORO
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Data: Dec 22, 2022
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Show Abstract
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The shock tube is an equipment used in laboratory studies on supersonic flows, providing data on the flight conditions in which the aerospace vehicles will find themselves. The Federal University of Rio Grande do Norte (UFRN) has stainless steel tubes – donated by the Institute of Advanced Studies (IEAv) – intended for the construction of the Institution's first shock tube. The objective of the research carried out was to make the construction of the equipment technically feasible. The correct sizing of the components is a fundamental part of the project, being essential to prevent accidents and control measurement errors during the tests, since it is a device subjected to high pressures. Structural modeling through software allows reducing material waste and operational risks during the construction of prototypes. Boundary conditions and applied loads must be rigorously selected, to provide a good level of confidence to the research results and, thus, constitute a guide for the execution of the academic project in a technical way. For this, the following were carried out and are presented here: calculations of the flow conditions; modeling and structural analysis of the high pressure (driver) and low pressure (driven) sections of the academic shock tube, considering the dimensions of the stainless steel tubes available at UFRN; in addition to determining the efforts to which the tubes will be submitted when the equipment becomes operational. Analytical (Lamé Equations) and numerical (Ansys Mechanical) results of circumferential, radial and von Mises stresses were compared by means of their percentage variations. Autodesk Inventor was also used for simulations and comparisons with Ansys Mechanical results. Both the driver and the driven were analyzed considering their ends closed by means of flanges and thus treated as pressure vessels. Ansys Mechanical and Autodesk Inventor software were used in the analysis, with discretization of the models by mesh generation and application of the Finite Element Method. A pressure of 70 atm (7.09 MPa) was applied to the inner surface of the high pressure section during calculations and computer simulation, while other pressures generated in the flow were calculated and applied to the low pressure section. All pressures were also multiplied by four to assess the impact of this change in stresses. Based on the results obtained for von Mises stresses, circumferential stresses, and radial stresses, it was found that, considering the properties of stainless steel AISI 304 and steel SAE 4140, the available tubes will withstand the workloads within the operating range to which they will be subjected without implying any risk of damage, in view of the first stage of the UFRN academic shock tube construction project.
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