Caracterização de uso e cobertura da terra na Amazônia utilizando imagens duais multitemporais do COSMO-SkyMed

A utilização de imagens de radar é fonte alternativa de informações para subsidiar o monitoramento da região amazônica, visto que as imagens ópticas têm limitações de imageamento em zonas tropicais face a ocorrência de nuvens. Por conseguinte este trabalho teve como objetivo analisar a capacidade das imagens-radar de banda X multitemporais e polarizadas obtidas pelo satélite COSMO-SkyMed (COnstellation of small Satellites for Mediterranean basin Observation), no modo intensidade, isoladamente e agregados às informações texturais, na caracterização temática de uso e cobertura da terra no município de Humaitá/AM. A metodologia empregada consistiu da: análise das imagens duais obtidas em duas aquisições subsequentes, de forma a explorar a potencialidade do conjunto de dados na forma quad-pol intensidade; extração dos atributos texturais a partir da matriz de coocorrência (Gray Level Co-occurrence Matrix) e posterior classificação contextual; avaliação estatística de desempenho temático das imagens intensidade e texturais, isoladas e em grupos polarizados. Dentre os vários resultados alcançados, foi verificado que o grupo formado somente pelas imagens intensidade apresentou o melhor desempenho, comparado àqueles contendo os atributos texturais. Nesta separabilidade, estavam envolvidas as classes de floresta, floresta aluvial, reflorestamento, savana, pasto e queimada, obtendo-se 66% de acurácia total e valor Kappa de 0,55. Os resultados mostraram que as imagens de banda X do COSMO-SkyMed, modo StripMap (Ping-Pong), multipolarizadas, têm potencial moderado para a caracterização e monitoramento da dinâmica de uso e cobertura da terra na Amazônia brasileira.

Taxa de absorção atmosférica sobre as cidades de Botucatu-SP e Rio de Janeiro-RJ

O segundo satélite da Missão Espacial Completa Brasileira (SCD2/MECB) foi colocado em órbita em 23 de Outubro de 1998 e carrega a bordo um experimento de células solares. Célula solar de silício é um dispositivo semicondutor, que pode medir a intensidade da radiação visível e parte da radiação infravermelha (400-1100 nm). O experimento permite medir simultaneamente a insolação direta e parte da radiação solar que é refletida pela Terra para o espaço. Os dados do experimento célula solar são transmitidos em tempo real pela telemetria do satélite e recebidos pela estação terrestre em Cuiabá, MT-Brasil (16°S; 56°W). Este fato limita a cobertura espacial para um círculo sobre a América do Sul. O albedo planetário é obtido dentro desta cobertura e seus valores podem ser agrupados em períodos temporais (anual, sazonal ou mensal), ou podem ser estudados para várias localizações (latitude e longitude) durante a vida do satélite. O coeficiente de transmissão atmosférica ou índice de claridade (Kt), medido em estações meteorológicas na superfície da Terra, junto com o valor medido simultaneamente do albedo planetário, permite calcular o coeficiente de absorção atmosférica (Ka). O método desenvolvido neste trabalho para avaliar Ka considera que o albedo planetário é composto por duas partes: uma refletividade local e uma refletividade não local. Considerando este novo conceito, é definida uma taxa de absorção atmosférica (denominada Ra) que é a razão entre Ka e a potência de irradiância solar líquida, que não atravessou a atmosfera (100%-Kt). A taxa de absorção atmosférica assim definida é independente da cobertura de nuvens. O histograma de freqüência de Ra mostra os valores de 0,86±0,07 e 0,88±0,09 sobre as cidades de Botucatu-SP e do Rio de Janeiro-RJ, durante os anos de 1999 até 2006, respectivamente.

Short Lyapunov time: a method for identifying confined chaos

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Gravitational effects of Nix and Hydra in the external region of the Pluto-Charon system

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Analysing the new Saturnian rings, R/2004 S1 and R/2004 S2

The Cassini-Huygens arrival into the Saturnian system brought a large amount of data about the satellites and rings. Two diffuse rings were found in the region between the A ring and Prometheus. R/2004 S1 is coorbital to Atlas and R/2004 S2 is close to Prometheus. In this work we analysed the closest approach between Prometheus and both rings. As a result we found that the satellite removes particles from R/2004 S2 ring. Long-term numerical simulations showed that some particles can cross the F ring region . The well known region of the F ring, where small satellites are present and particles are being taking from the ring, gains a new insight with the presence of particles from R/2004 S2 ring. The computation of the Lyapunov Characteristic Exponent reveled that the R/2004 S2 ring lies in a chaotic region while R/2004 S1 ring and Atlas are in a stable region. Atlas is responsible for the formation of three regimes in the R/2004 S1 ring, as expected for a satellite embedded in a ring.

Dynamical capture in the Pluto-Charon system

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Feeding patterns in a fish community of Baia da Onça, a floodplain lake of the Aquidauana River, Pantanal, Brazil

The stomach contents of 24 species of fish and unidentified species from four genera in a floodplain lake of the Pantanal were studied. Fish were collected during the dry season when the lake was isolated from the main river. A community food ingestion index (feeding index weighted by consumer biomass, FIWCB, where 0 < FIWCB < 1) was calculated to quantify feeding patterns. Detritus and algae ingested by Curimatidae were responsible for 46.5% of the FIWCB, while that for algae ingested by Loricariidae (armoured catfish) accounted for 13.2%. The importance of detritus in fish diets is discussed as a strategy for shortening food chains, thereby increasing community efficiency, and as a consequence, fish biomass. It was learnt that the main route of energy flow in this perennial lake was through the detritus chain. The floodplain lakes function as a dry season feeding ground for small-sized species of fish, which are potential prey for the more highly valued larger species of fish.

As usinas hidrelétricas e seus impactos: os aspectos socioambientais e econômicos do reassentamento rural de Rosana-Euclides da Cunha Paulista

Pós-graduação em Geografia - FCT

Dinâmica do sistema binário Plutão-Caronte

Pós-graduação em Física - FEG

Long-term dynamics of Methone, Anthe and Pallene

We numerically investigate the long-term dynamics of the Saturn's small satellites Methone (S/2004 S1), Anthe (S/2007 S4) and Pallene (S/2004 S2). In our numerical integrations, these satellites are disturbed by non-spherical shape of Saturn and the six nearest regular satellites. The stability of the small bodies is studied here by analyzing long-term evolution of their orbital elements.We show that long-term evolution of Pallene is dictated by a quasi secular resonance involving the ascending nodes (12) and longitudes of pericentric distances (pi) of Mimas (subscript 1) and Pallene (subscript 2), which critical argument is pi(2) - pi(1) - Omega(1) + Omega(2) Long-term orbital evolution of Methone and Anthe are probably chaotic since: i) their orbits randomly cross the orbit of Mimas in time scales of thousands years); ii) long-term numerical simulations involving both small satellites are strongly affected by small changes in the initial conditions.

The evolution of a Pluto-like system during the migration of the ice giants

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Nonlinear Control of Magnetically Actuated Spacecraft

The topic of this thesis is the feedback stabilization of the attitude of magnetically actuated spacecraft. The use of magnetic coils is an attractive solution for the generation of control torques on small satellites flying inclined low Earth orbits, since magnetic control systems are characterized by reduced weight and cost, higher reliability, and require less power with respect to other kinds of actuators. At the same time, the possibility of smooth modulation of control torques reduces coupling of the attitude control system with flexible modes, thus preserving pointing precision with respect to the case when pulse-modulated thrusters are used. The principle based on the interaction between the Earth's magnetic field and the magnetic field generated by the set of coils introduces an inherent nonlinearity, because control torques can be delivered only in a plane that is orthogonal to the direction of the geomagnetic field vector. In other words, the system is underactuated, because the rotational degrees of freedom of the spacecraft, modeled as a rigid body, exceed the number of independent control actions. The solution of the control issue for underactuated spacecraft is also interesting in the case of actuator failure, e.g. after the loss of a reaction-wheel in a three-axes stabilized spacecraft with no redundancy. The application of well known control strategies is no longer possible in this case for both regulation and tracking, so that new methods have been suggested for tackling this particular problem. The main contribution of this thesis is to propose continuous time-varying controllers that globally stabilize the attitude of a spacecraft, when magneto-torquers alone are used and when a momentum-wheel supports magnetic control in order to overcome the inherent underactuation. A kinematic maneuver planning scheme, stability analyses, and detailed simulation results are also provided, with new theoretical developments and particular attention toward application considerations.

Enhancement of Trajectory Determination of Orbiter Spacecraft by Using Pairs of Planetary Optical Images

The subject of the present thesis is about the enhancement of orbiter spacecraft navigation capabilities obtained by the standard radiometric link, taking advantage of an imaging payload and making use of a novel definition of optical measurements. An ESA Mission to Mercury called BepiColombo, was selected as a reference case for this study, and in particular its Mercury Planetary Orbiter (MPO), because of the presence of SIMBIO-SYS, an instrument suite part of the MPO payload, capable of acquiring high resolution images of the surface of Mercury. The use of optical measurements for navigation, can provide complementary informations with respect to Doppler, for enhanced performances or a relaxation of the radio tracking requisites in term of ground station schedule. Classical optical techniques based on centroids, limbs or landmarks, were the base to a novel idea for optical navigation, inspired by concepts of stereoscopic vision. In brief, the relation between two overlapped images acquired by a nadir pointed orbiter spacecraft at different times, was defined, and this information was then formulated into an optical measurement, to be processed by a navigation filter. The formulation of this novel optical observable is presented, moreover the analysis of the possible impact on the mission budget and images scheduling is addressed. Simulations are conducted using an orbit determination software already in use for spacecraft navigation in which the proposed optical measurements were implemented and the final results are given.

Biogenic volatile organic compounds in tropical, temperate and boreal forest ecosystems

Biogene flüchtige organische Verbindungen (BFOV) werden in großen Mengen aus terrestrischenrnÖkosystemen, insbesondere aus Wäldern und Wiesen, in die untere Troposphäre emittiert. Austausch-rnFlüsse von BFOVs sind in der troposphärischen Chemie wichtig, weil sie eine bedeutende Rolle in derrnOzon- und Aerosolbildung haben. Trotzdem bleiben die zeitliche und räumliche Änderung der BFOVrnEmissionen und ihre Rolle in Bildung und Wachstum von Aerosolen ungewiss.rnDer Fokus dieser Arbeit liegt auf der in-situ Anwendung der Protonen Transfer ReaktionsrnMassenspektrometrie (PTR-MS) und der Messung von biogenen flüchtigen organischen Verbindungen inrnnordländischen, gemäßigten und tropischen Waldökosystemen während drei unterschiedlicherrnFeldmesskampagnen. Der Hauptvorteil der PTR-MS-Technik liegt in der hohen Messungsfrequenz,rnwodurch eine eventuelle Änderung in der Atmosphäre durch Transport, Vermischung und Chemiernonline beobachtet werden kann. Die PTR-MS-Messungen wurden zweimal am Boden aus und einmalrnvon einem Forschungsflugzug durchgeführt.rnIn Kapitel 3 werden die PTR-MS-Daten, gesammelt während der Flugmesskampagne über demrntropischen Regenwald, vorgelegt. Diese Studie zeigt den Belang der Grenzschichtdynamik für diernVerteilung von Spurengasen mittels eines eindimensionalen Säule - Chemie und KlimaModells (SCM).rnDer Tagesablauf von Isopren zeigte zwischen 14:00 und 16:15 Uhr lokaler Zeit einen Mittelwert vonrn5.4 ppbv auf der Höhe der Baumspitzen und von 3.3 ppbv über 300 m Höhe. Dies deutet darauf hin, dassrnsowohl der turbulente Austausch als auch die hohe Reaktionsfähigkeit von Isopren mit den OxidantienrnOH und Ozon eine wichtige Rolle spielen. Nach dem Ausgleich von chemischen Verlusten undrnEntrainment (Ein- und Ausmischung von Luft an der Grenzschicht), wurde ein Fluss vonrn8.4 mg Isopren m-2h-1 unter teilweise bewölkten Bedingungen für den tropischen Regenwald in derrnGuyanregion abgeschätzt. Dies entspricht einem täglichen Emissionsfluss von 28 mg Isopren prornQuadratmeter.rnIm Kapitel 4 werden die Messungen, welche auf einer Hügellage in gemäßigter Breite inrnsüddeutschland stattgefunden haben, diskutiert. Bei diesem Standort ist die Grenzschicht nachts unter diernStandorthöhe abgefallen, was den Einsatzort von Emissionen abgesondert hatte. Während diernGrenzschicht morgens wieder über die Höhe des Einsatzortes anstieg, konnten die eingeschlossenenrnnächtlichen Emissionen innerhalb der bodennahen Schicht beobachtet werden. Außerdem wurde einrndeutlicher Anstieg von flüchtigen organischen Verbindungen gemessen, wenn die Luftmassen überrnMünchen geführt wurden oder wenn verschmutzte Luftmassen aus dem Po-Tal über die Alpen nachrnDeutschland transportiert wurden. Daten von dieser Kampagne wurden genutzt, um die Änderungen inrndem Mischungsverhältnis der flüchtigen organischen Verbindungen, verbunden mit dem Durchfluss vonrnwarmen und kalten Wetterfronten sowie bei Regen zu untersuchen.rnIm Kapitel 5 werden PTR-MS-Messungen aus dem nördlichen Nadelwaldgürtel beschrieben. Starkernnächtliche Inversionen mit einer niedrigen Windgeschwindigkeit fingen die Emissionen vonrnnahegelegenen Kiefernwäldern und andere BFOV-Quellen ab, was zu hohen nächtlichen BFOVMischverhältnissenrnführte. Partikelereignisse wurden für Tag und Nacht detailliert analysiert. Diernnächtlichen Partikelereignisse erfolgten synchron mit starken extremen von Monoterpenen, obwohl dasrnzweite Ereignis Kernbildung einschloss und nicht mit Schwefelsäure korrelierte. Die MonoterpenrnMischungsverhältnisse von über 16 ppbv waren unerwartet hoch für diese Jahreszeit. NiedrigernWindgeschwindigkeiten und die Auswertung von Rückwärtstrajektorien deuten auf eine konzentrierternQuelle in der Nähe von Hyytiälä hin. Die optische Stereoisomerie von Monoterpenen hat bestätigt, dassrndie Quelle unnatürlich ist, da das Verhältnis von [(+)-α-pinen]/[(−)-α-pinen] viel höher ist als dasrnnatürliches Verhältnis der beiden Enantiomeren.

Progettazione della sala di controllo missione della stazione di ricetrasmissione satellitare di Forlì

In questo lavoro di tesi si è voluto rappresentare, mediante l'utilizzo del software SolidWorks, quella che sarà la nuova stazione di ricetrasmissione satellitare di Forlì, già esistente presso il laboratorio di radioscienza ed esplorazione planetaria sotto il nome di Alma Mater Ground Station (AMGS), la quale lavorerà come sala di controllo missione nel nuovo progetto della European Space Agency (ESA), ovvero la missione ESEO, progetto educativo che vede il contributo di studenti provenienti da varie facoltà europee. È stato inizialmente ampliato il lavoro di tirocinio svolto dal candidato, il quale ha riguardato la rappresentazione in SolidWorks delle antenne che saranno utilizzate dalla stazione di ricetrasmissione e del loro futuro posizionamento, mediante uno studio strutturale dei tralicci che sosterranno le antenne, quindi ponendo attenzione al carico del vento al quale potrà essere sottoposta l'antenna parabolica del diametro di 3 metri. Successivamente è stato svolto uno studio generale dell'attrezzatura necessaria alla comunicazione satellitare,e quindi dell'interconnessione dei vari componenti. Quindi è stata disegnata in SolidWorks la sala di controllo missione, che sarà ubicata presso il nuovo tecnopolo che sorgerà nelle vicinanze della Scuola di ingegneria, il quale sarà sede del CIRI Aeronautica, Spazio e Mobilità di Forlì. Sono state importate le antenne, già disegnate nel lavoro di tirocinio, e sono stati disegnati i vari componenti e arredamenti della sala di controllo, disponendoli in modo tale da creare una visione vicina alla realtà.