Luminescence is the emission of light by an object. Living organisms including certain bacteria are capable of luminescence. Bacteria are the most abundant luminescent organisms in nature. Bacterial luminescence has been studied most extensively in several marine bacteria. Bacterial luminescence is due to the action of the enzyme called luciferase. The luminescent bacteria exist in nature either as free living bacteria or in symbiotic association ship with certain marine organisms. Research on luminescent bacteria has always been a fascinating one. In the present study, twenty free living luminescent bacteria were isolated from Bay of Bengal, India using soft agar overlay method in sea water complex agar (SWCA). All the 20 strains were characterized for certain biochemical tests and they were tentatively identified that they are all Photobacterium spp. The effect of salinity, pH glycerol concentration and heavy metals on the growth and luminescence of these 20 strains was also studied. In this part of experiment, visual scoring was done to categorize the luminescence. In case of salinity, it has been found that up to 6% of NaCl the intense of luminescence was good and thereafter it declined. Further, in some strains it was completely ceased beyond 9% of salinity. Luminescence was not greatly affected by pH in liquid medium however; the same was affected in solid medium. The intensity of luminescence has increased with increasing concentrations of glycerol ranging from 0.3 to 1.2%. All the 20 luminescent bacteria were characterized for their tolerance to heavy metals and antibiotics. Copper and zinc at 1 mg/ml concentration have inhibited the growth and luminescence of the all strains. Surprisingly, mercury at the same concentration has inhibited only two strains (AMET1913 and AMET1920). However, at 2 mg/ml concentration mercury has inhibited the growth and luminescence of all the 20 strains. Selected six luminescent bacterial strains were also characterized for their antibiotic susceptibility against six different antibiotics. It has been found that most of the strains were sensitive to all the six antibiotics tested. Since, the bioluminescence is regulated by quorum sensing, the effect of culture filtrate extracted with dichloromethane was also tested for its effect on luminescence. These DCM extracts haven‟t influenced the luminescence much.

Myanmar remained largely closed to the world through political instability for several years, when it continued to suffer terribly at the hands of nature that remained largely unknown. Of note is the period between 2008 and 2013, during which the country suffered at least eight major natural calamities that killed more than 141,000 people and affected 3.2 million. The worst of these was Cyclone Nargis in May 2008 that killed more than 130,000. With an estimated $4 billion in damages, Nargis remains the deadliest and most destructive named cyclone ever to have occurred in the North Indian Ocean. Recent studies have shown that, due to increased greenhouse gases and aerosol loading in the atmosphere, more and stronger tropical cyclones (TCs) in the last three decades are tracking eastwards toward the Indochina peninsula. Unfortunately, the Burmese lack the capacity to deal with the impacts of such storms. Myanmar was left behind as the world made significant technological and industrial advancement; but agriculture, which employs at least 65% of the active labor force, has remained the backbone of the Myanmar economy – an industry that is heavily reliant on monsoon rainfall. The pre-monsoon TC season in the Bay of Bengal (BoB) precedes the onset of the Myanmar monsoon but sometimes the two (i.e.TC formation and the monsoon onset) occur in unison. This work studied the mechanism by which the Madden Julian Oscillation (MJO) modulates the Myanmar monsoon onset and TC activity collectively (i.e. ISO-Onset-TC connection). Avoiding TC destruction at the beginning of the planting season is crucial, so is the monsoon onset date critical for planning. Additional understanding of the aforementioned ISO-Onset-TC connection could provide further insight into predicting the Myanmar monsoon onset and aid in disaster planning for TC impact. This research is part of a two-year NASA funded project to study extreme climate and weather events.

No description available.

Geochemical processes associated with gas hydrate formation lead to the growth of iron sulphides which have a geophysically-measurable magnetic signature. Detailed magnetic investigation, complemented by petrological observations, were undertaken on cores from a permafrost setting, the Mackenzie Delta (Canadian Northwest Territories) Mallik region, and two marine settings, IODP Expedition 311 cores from the Cascadia margin off Vancouver Island and the Indian National Gas Hydrate Program Expedition 1 from the Bengal Fan. Stratigraphic profiles of the fine scale variations in bulk magnetic measurements correspond to changes in lithology, grain size and pore fluid geochemistry which can be correlated on local to regional scales. The lowest values of magnetic susceptibility are observed where iron has been reduced to paramagnetic pyrite, formed in settings with high methane and sulphate or sulphide flux, such as at methane vents. High magnetic susceptibility values are observed in sediments which contain detrital magnetite, for example from glacial deposits, which has survived diagenesis. Other high magnetic susceptibility values are observed in sediments in which the ferrimagnetic iron-sulphide minerals greigite or smythite have been diagenetically introduced. These minerals are mostly found outside the sediments which host gas hydrate. The mineral textures and compositions indicate rapid disequilibrium crystallization. The unique physical and geochemical properties of the environments where gas hydrates form, including the availability of methane to fuel microbiological activity and the concentration of pore water solutes during gas hydrate formation, lead to iron sulphide precipitation from solute-rich brines. Magnetic surveying techniques help delineate anomalies related to gas hydrate deposits and the diagenesis of magnetic iron minerals related to their formation. Detailed core logging measurements and laboratory analyses of magnetic properties provide direct ties to original lithology, petrophysical properties and diagenesis caused by gas hydrate formation.

No description available.

Le Golfe du Bengale (GdB), dans l'océan indien Nord, est sous l'influence d'intenses vents de mousson, qui se renversent saisonnièrement. Les fortes pluies et les apports fluviaux associés à la mousson de Sud-Ouest font du GdB l'une des régions les moins salées des océans tropicaux. La forte stratification haline proche de la surface qui en découle contribue à limiter le mélange vertical, ce qui maintient des températures de surface élevées et favorise la convection atmosphérique et les pluies. Cette stratification en sel a ainsi des implications profondes sur les échanges air-mer et sur le climat des pays riverains. L'objectif de ma thèse est d'améliorer la description de la variabilité de la salinité de surface (SSS) du GdB, et de comprendre ses mécanismes aux échelles de temps saisonnières à interannuelles. Les climatologies existantes ont permis de mettre en évidence un cycle saisonnier marqué de la SSS, avec un dessalement intense de la partie Nord du bassin pendant l'automne, suivi par une expansion de ces eaux dessalées le long du bord Ouest du bassin. Cette langue dessalée s'érode finalement pendant l'hiver, pour revenir à son extension minimale au printemps. Cependant, la rareté des observations in-situ de SSS ne permet d'observer les fluctuations interannuelles autour de ce cycle saisonnier que de manière parcellaire dans le GdB. Le développement récent de la télédétection spatiale de la SSS (missions SMOS et AQUARIUS) a ouvert de nouvelles opportunités à cet égard. Cette technologie reste toutefois délicate dans le cas d'un bassin de petite taille tel que le GdB, du fait des contaminations éventuelles du signal de SSS par les interférences radio et par les sources d'origine continentale. Une validation systématique des produits satellites par comparaison à un jeu de données in-situ exhaustif montre qu'Aquarius capture de façon réaliste les évolutions saisonnières et interannuelles de la SSS partout dans le GdB. A l'inverse, SMOS ne parvient pas à restituer une salinité meilleure que les climatologies existantes. / Located in the Northern Indian Ocean, the Bay of Bengal (BoB) is forced by intense seasonally reversing monsoon winds. Heavy rainfall and strong river runoffs associated with the southwest monsoon makes the bay one of the freshest regions in the tropical ocean. This surface fresh water flux induces strong near surface salinity stratification, which reduces vertical mixing and maintains high sea surface temperatures and deep atmospheric convection and rainfall. This intense near surface haline stratification has therefore profound implications on the air-sea exchanges, and on the climate of the neighboring countries. The goal of my thesis is to improve the description of the Sea surface salinity (SSS) variability in the BoB and to understand the oceanic and atmospheric processes driving this variability at seasonal and interannual timescales. Existing climatologies reveal a marked seasonal cycle of SSS with an intense freshening of the northern part of the basin during fall that subsequently spreads along the western boundary. This fresh pool finally erodes during winter, to reach its minimal extent in spring. The paucity of in-situ SSS observations however prevented to monitor the interannual fluctuations around this seasonal picture with a good spatial coverage. The recent development of SSS remote-sensing capabilities (with SMOS and AQUARIUS satellites) may help with that regard. However this is particularly challenging for a small semi-enclosed basin such as the Bay of Bengal, because of the potential contamination of the SSS signal by radio frequency interferences and land effects in the near coastal environment. A thorough validation of these satellite products to an exhaustive gridded in-situ dataset shows that Aquarius reasonably captures the large-scale observed seasonal and interannual SSS evolution everywhere in the BoB while SMOS does not perform better than existing climatologies, advocating for improvements of its SSS retrieval algorithm there.

Recent years witnessed a vast advent of stalagmites as palaeoclimate archives. The multitude of geochemical and physical proxies and a promise of a precise and accurate age model greatly appeal to palaeoclimatologists. Although substantial progress was made in speleothem-based palaeoclimate research and despite high-resolution records from low-latitudinal regions, proving that palaeo-environmental changes can be archived on sub-annual to millennial time scales our comprehension of climate dynamics is still fragmentary. This is in particular true for the summer monsoon system on the Indian subcontinent. The Indian summer monsoon (ISM) is an integral part of the intertropical convergence zone (ITCZ). As this rainfall belt migrates northward during boreal summer, it brings monsoonal rainfall. ISM strength depends however on a variety of factors, including snow cover in Central Asia and oceanic conditions in the Indic and Pacific. Presently, many of the factors influencing the ISM are known, though their exact forcing mechanism and mutual relations remain ambiguous. Attempts to make an accurate prediction of rainfall intensity and frequency and drought recurrence, which is extremely important for South Asian countries, resemble a puzzle game; all interaction need to fall into the right place to obtain a complete picture. My thesis aims to create a faithful picture of climate change in India, covering the last 11,000 ka. NE India represents a key region for the Bay of Bengal (BoB) branch of the ISM, as it is here where the monsoon splits into a northwestward and a northeastward directed arm. The Meghalaya Plateau is the first barrier for northward moving air masses and receives excessive summer rainfall, while the winter season is very dry. The proximity of Meghalaya to the Tibetan Plateau on the one hand and the BoB on the other hand make the study area a key location for investigating the interaction between different forcings that governs the ISM. A basis for the interpretation of palaeoclimate records, and a first important outcome of my thesis is a conceptual model which explains the observed pattern of seasonal changes in stable isotopes (d18O and d2H) in rainfall. I show that although in tropical and subtropical regions the amount effect is commonly called to explain strongly depleted isotope values during enhanced rainfall, alone it cannot account for observed rainwater isotope variability in Meghalaya. Monitoring of rainwater isotopes shows no expected negative correlation between precipitation amount and d18O of rainfall. In turn I find evidence that the runoff from high elevations carries an inherited isotopic signature into the BoB, where during the ISM season the freshwater builds a strongly depleted plume on top of the marine water. The vapor originating from this plume is likely to memorize' and transmit further very negative d18O values. The lack of data does not allow for quantication of this plume effect' on isotopes in rainfall over Meghalaya but I suggest that it varies on seasonal to millennial timescales, depending on the runoff amount and source characteristics. The focal point of my thesis is the extraction of climatic signals archived in stalagmites from NE India. High uranium concentration in the stalagmites ensured excellent age control required for successful high-resolution climate reconstructions. Stable isotope (d18O and d13C) and grey-scale data allow unprecedented insights into millennial to seasonal dynamics of the summer and winter monsoon in NE India. ISM strength (i. e. rainfall amount) is recorded in changes in d18Ostalagmites. The d13C signal, reflecting drip rate changes, renders a powerful proxy for dry season conditions, and shows similarities to temperature-related changes on the Tibetan Plateau. A sub-annual grey-scale profile supports a concept of lower drip rate and slower stalagmite growth during dry conditions. During the Holocene, ISM followed a millennial-scale decrease of insolation, with decadal to centennial failures resulting from atmospheric changes. The period of maximum rainfall and enhanced seasonality corresponds to the Holocene Thermal Optimum observed in Europe. After a phase of rather stable conditions, 4.5 kyr ago, the strengthening ENSO system dominated the ISM. Strong El Nino events weakened the ISM, especially when in concert with positive Indian Ocean dipole events. The strongest droughts of the last 11 kyr are recorded during the past 2 kyr. Using the advantage of a well-dated stalagmite record at hand I tested the application of laser ablation-inductively coupled plasma-mass spectrometry (LA-ICP-MS) to detect sub-annual to sub-decadal changes in element concentrations in stalagmites. The development of a large ablation cell allows for ablating sample slabs of up to 22 cm total length. Each analyzed element is a potential proxy for different climatic parameters. Combining my previous results with the LAICP- MS-generated data shows that element concentration depends not only on rainfall amount and associated leaching from the soil. Additional factors, like biological activity and hydrogeochemical conditions in the soil and vadose zone can eventually affect the element content in drip water and in stalagmites. I present a theoretical conceptual model for my study site to explain how climatic signals can be transmitted and archived in stalagmite carbonate. Further, I establish a first 1500 year long element record, reconstructing rainfall variability. Additionally, I hypothesize that volcanic eruptions, producing large amounts of sulfuric acid, can influence soil acidity and hence element mobilization. / Stalagmiten erfuhren in den letzten Jahren vermehrt Aufmerksamkeit als bedeutende Paläoklima- Archive. Paläoklimatologen sind beeindruckt von der grossen Zahl geochemischer und physikalischer Indikatoren (Proxies) und der Möglichkeit, präzise absolute Altersmodelle zu erstellen. Doch obwohl substantielle Fortschritte in der speleothem-basierten Klimaforschung gemacht wurden, und trotz hochaufgelöster Archive aus niederen Breiten, welche zeigen, das Umweltveränderungen auf Zeitskalen von Jahren bis Jahrtausenden archiviert und rekonstruiert werden können, bleibt unser Verständnis der Klimadynamik fragmentarisch. Ganz besonders gilt dies für den Indischen Sommermonsun (ISM) auf dem Indischen Subkontinent. Der ISM ist heute als ein integraler Bestandteil der intertropischen Konvergenzzone verstanden. Sobald dieser Regengürtel während des borealen Sommer nordwärts migriert kann der ISM seine feuchten Luftmassen auf dem Asiatischen Festland entladen. Dabei hängt die Stärke des ISM von einer Vielzahl von Faktoren ab. Zu diesen gehören die Schneedicke in Zentralasien im vorhergehenden Winter und ozeanische Bedingungen im Indischen und Pazifschen Ozean. Heute sind viele dieser Faktoren bekannt. Trotzdem bleiben deren Mechanismen und internen Verbindungen weiterhin mysteriös. Versuche, korrekte Vorhersagen zu Niederschlagsintensität und Häufigkeit oder zu Dürreereignissen zu erstellen ähneln einem Puzzle. All die verschiedenen Interaktionen müssen an die richtige Stelle gelegt werden, um ein sinnvolles Bild entstehen zu lassen. Meine Dissertation versucht, ein vertrauenswürdiges Bild des sich wandelnden Holozänen Klimas in Indien zu erstellen. NE Indien ist eine Schlüsselregion für den östlichen Arm des ISM, da sich hier der ISM in zwei Arme aufteilt, einen nordwestwärts und einen nordostwärts gerichteten. Das Meghalaya Plateau ist das erste Hindernis für die sich nordwärts bewegenden Luftmassen und erhält entsprechend exzessive Niederschläge während des Sommers. Die winterliche Jahreszeit dagegen ist sehr trocken. Die Nähe zum Tibetplateau einerseits und der Bucht von Bengalen andererseits determinieren die Schlüsselposition dieser Region für das Studium der Interaktionen der den ISM beeinflussenden Kräfte. Ein Fundament für die Interpretation der Paläoklimarecords und ein erstes wichtiges Ergebnis meiner Arbeit ist ein konzeptuelles Modell, welches die beobachteten saisonalen Veränderungen stabiler Isotope (d18O und d2H) im Niederschlag erklärt. Ich zeige, das obwohl in tropischen und subtropischen Regionen meist der amount effect zur Erklärung stark negativer Isotopenwerte während starker Niederschläge herangezogen wird, dieser allein nicht ausreicht, um die Isotopenvariabilität im Niederschlag Meghalaya's zu erklären. Die Langzeitbeobachtung der Regenwasserisotopie zeigt keine negative Korrelation zwischen Niederschlagsmenge und d18O. Es finden sich Hinweise, das der Abfluss aus den Hochgebirgsregionen Tibets und des Himalaya eine Isotopensignatur an das Oberflächenwasser der Bucht von Bengalen vererbt. Dort bildet sich aus isotopisch stark abgereicherten Wässern während des ISM eine Süsswasserlinse aus. Es ist wahrscheinlich, das Wasserdampf, der aus dieser Linse stammt, ein Isotopensignal aufgeprägt bekommt, welches abgereichertes d18O weitertransportiert. Der Mangel an Daten lässt es bisher leider nicht zu, quantitative Aussagen über den Einfluss dieses plume effect' auf Niederschläge in Meghalaya zu treffen. Es lässt sich allerdings vermuten, das dieser Einfluss auf saisonalen wie auch auf langen Zeitskalen variabel ist, abhängig vom Abfluss und der Quellencharacteristik. Der Fokus meiner Arbeit liegt in der Herauslösung klimatischer Signale aus nordostindischen Stalagmiten. Hohe Urankonzentrationen in diesen Stalagmiten erlaubt eine exzellente Alterskontrolle, die für hochauflösende Klimarekonstruktionen unerlässlich ist. Die stabilen Isotope (d18O und d13C), sowie Grauwertdaten, erlauben einmalige Einblicke in die Dynamik des Sommer und auch des Wintermonsun in NE Indien. Die ISM Stärke (d. h. Niederschlagsmenge) wird in Veränderungen in den d18Ostalagmites reflektiert. Das d13C Signal, welches Tropfratenänderungen speichert, dient als potenter Indikator für winterliche Trockenheitsbedingungen. Es zeigt Ähnlichkeit zu temperaturabhängigen Veränderungen auf dem Tibetplateau. Das sub-annuell aufgelöste Grauwertprofil stärkt das Konzept, das verminderte Tropfraten und langsameres Stalagmitenwachstum eine Folge von Trockenheit sind. Während des Holozäns folgte der ISM der jahrtausendelangen Verringerung der Insolation. Es finden sich aber ebenso rapide Anomalien, die aus atmosphärischen Veränderungen resultieren. Die Phase des höchsten Niederschlages und erhöhter Saisonalität korrespondiert mit dem Holozänen Thermalen Maximum. Nach einer Phase einigermassen stabilen Bedingungen begann vor ca. 4500 Jahren ENSO einen zunehmenden Einfluss auf den ISM auszuüben. Starke El Nino Ereignisse schwächen den ISM, besonders wenn diese zeitgleich mit positiven Indian Ocean Dipole Ereignissen auftreten. Die stärksten Dürren des gesamten Holozäns traten in den letzten 2000 Jahren auf. Um zusätzliche Informationen aus den hervorragenden Proben zu gewinnen nutzte ich die Vorteile der laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS). Diese erlaubt die Detektion sub-annueller bis sub-dekadischer Elementkonzentrationsveränderungen in Stalagmiten. Mittels einer neu entwickelten Ablationszelle konnten Proben von maximal 22 cm Länge untersucht werden. Jedes analysierte Element ist ein potentieller Träger einer Klimainformation. Die Kombination der früheren Ergebnisse mit denen der LA-IPC-MS zeigt, das die Elementkonzentrationen nicht nur von Niederschlagsveränderungen und assoziiertem Auswaschen aus dem Boden abhängen. Zusätzlich können auch die biologische Aktivität und hydrogeochemische Bedingungen in der vadosen Zone Einfluss auf die Elementzusammensetzung im Tropfwasser und in den Stalagmiten haben. Darum entwickelte ich ein theoretisches Modell für meinen Standort, um zu klären, wie Klimasignale von der Atmosphäre in die Höhle transportiert werden können. Ein anschliessend rekonstruierter 1500 Jahre langer Proxyrecord zeigt Niederschlagsvariabilität an. Zudem besteht die Möglichkeit, das Vulkaneruptionen, welche grosse Mengen an Schwefelsäure produzieren, eine Bodenversauerung verursachen und damit die Elementmobilisierung verstärken können.

A bacia de Bengala, localizada a Nordeste da Índia tem uma história evolutiva extraordinária, diretamente controlada bela fragmentação do Gondwana. O início da formação desta bacia é considerada como sendo relacionada ao final do evento da quebra, datado em 126 Ma quando a Índia separou do continente Antártico e da Austrália. Desde então, a placa continental Indiana viajou do pólo sul a uma velocidade muito rápida (16 cm/a) chocando-se com o hemisfério norte e fundindo-se com a Placa Eurasiana. Durante a viagem passou por cima de um hot spot, onde hoje estão localizadas as ilhas Seicheles, resultando em um dos maiores derrames de lava basáltica do mundo, conhecido como Deccan Trap. Na região onde a bacia de Bengala foi formada, não houve aporte significativo de sedimentos siliciclásticos, resultando na deposição de uma espessa plataforma carbonática do Cretáceo tardio ao Eoceno. Após este período, devido a colisão com algumas microplacas e a amalgamação com a Placa Eurasiana, um grande volume sedimentar siliciclástico foi introduzido para a bacia, associado também ao soerguimento da cadeia de montanhas dos Himalaias. Atualmente, a Bacia de Bengala possui mais de 25 km de sedimentos, coletados neste depocentro principal. Nesta dissertação foram aplicados conceitos básicos de sismoestratigrafia na interpretação de algumas linhas regionais. As linhas sísmicas utilizadas foram adquiridas recentemente por programa sísmico especial, o qual permitiu o imageamento sísmico a mais de 35km dentro da litosfera (crosta continental e transicional). O dado permitiu interpretar eventos tectônicos, como a presença dos Seawards Dipping Reflectors (SDR) na crosta transicional, coberto por sedimentos da Bacia de Bengala. Além da interpretação sísmica amarrada a alguns poços de controle, o programa de modelagem sedimentar Beicip Franlab Dionisos, foi utilizado para modelar a história de preenchimento da bacia para um período de 5,2 Ma. O nível relativo do nível do mar e a taxa de aporte sedimentar foram os pontos chaves considerados no modelo. Através da utilização dos dados sísmicos, foi possível reconhecer dez quebras de plataformas principais, as quais foram utilizadas no modelo, amarrados aos seus respectivos tempos geológico, provenientes dos dados dos poços do Plioceno ao Holoceno. O resultado do modelo mostrou que a primeira metade modelada pode ser considerada como um sistema deposicional retrogradacional, com algum picos transgressivos. Este sistema muda drasticamente para um sistema progradacional, o qual atuou até o Holoceno. A seção modelada também mostra que no período considerado o total de volume depositado foi em torno de 2,1 x 106 km3, equivalente a 9,41 x 1014 km3/Ma. / The Bengal Basin in Northeast India has a remarkable evolution history directly controled by the Gondwana fragmentation. The Beginning of this basin is considered related to the final break up event, dated as 126 Ma when India finally became separeted from Antarctica and Australia Continents. Since then, the India Continental Plate traveled from the South pole at very fast rate (16 cm/y) reaching the nortern hemisphere and merging with Eurasia Plate. During the travel it passed over a hot spot, located where is today Seychelles Island, resulting in one of the biggest basalt leakage, know as Deccan Trap. In the area where the Bengal Basin was formed during the travel there wasnt any supply of siliciclastics, resulting in the deposition of a very thick section of carbonate platforms from Late Cretaceous to Eocene. After this period, due to the collision with same microplates and the amalgamation with Eurasia Plate a huge siliciclastic supply was introduced in the basin, associated with rising of the Himalayas Mountains. Therefore, the Belgal Basin today has more than 25 km of sediments, collected in its main depocenter. In this dissertation it was applied to the basic concepts of seismostratigraphy in the interpretation of some regional lines. These seismic lines were acquired recently by a special survey program that allowed having good quality data until more than 35 km in the lithosphere (continental and transitional crust). The data permitted to interpret tectonic events such as the presence of Seawards Dipping Reflectors (SDR) in the transitional crust, covered by the Bengal Basin sediments. Besides the seismic interpretation tied to some well data, it was used in the dissertation a Beicip Franlab Software, known as Dionisos, to model and develop a basin fill history. The eustatic relative sea level flutuations and sediment rate of sediment influx are the key points to be considered in the model. Using the seismic data it was possible to recognize ten main platform breakes than were used in the model, tied to a geological time frame provided by the well data interpretation, from Pliocene to Holocene. The output of the model shown that a first half of the considered time predominated a major retrogradational system, with some minor trangression peaks. This changed to a very strong progradational system that is acting until the Holocene. The section modeled also shows a total of sediments deposited in the period considered was about 2,1 x106 km3 equivalent to a 9,41 x 1014 km3/Ma.

A bacia de Bengala, localizada a Nordeste da Índia tem uma história evolutiva extraordinária, diretamente controlada bela fragmentação do Gondwana. O início da formação desta bacia é considerada como sendo relacionada ao final do evento da quebra, datado em 126 Ma quando a Índia separou do continente Antártico e da Austrália. Desde então, a placa continental Indiana viajou do pólo sul a uma velocidade muito rápida (16 cm/a) chocando-se com o hemisfério norte e fundindo-se com a Placa Eurasiana. Durante a viagem passou por cima de um hot spot, onde hoje estão localizadas as ilhas Seicheles, resultando em um dos maiores derrames de lava basáltica do mundo, conhecido como Deccan Trap. Na região onde a bacia de Bengala foi formada, não houve aporte significativo de sedimentos siliciclásticos, resultando na deposição de uma espessa plataforma carbonática do Cretáceo tardio ao Eoceno. Após este período, devido a colisão com algumas microplacas e a amalgamação com a Placa Eurasiana, um grande volume sedimentar siliciclástico foi introduzido para a bacia, associado também ao soerguimento da cadeia de montanhas dos Himalaias. Atualmente, a Bacia de Bengala possui mais de 25 km de sedimentos, coletados neste depocentro principal. Nesta dissertação foram aplicados conceitos básicos de sismoestratigrafia na interpretação de algumas linhas regionais. As linhas sísmicas utilizadas foram adquiridas recentemente por programa sísmico especial, o qual permitiu o imageamento sísmico a mais de 35km dentro da litosfera (crosta continental e transicional). O dado permitiu interpretar eventos tectônicos, como a presença dos Seawards Dipping Reflectors (SDR) na crosta transicional, coberto por sedimentos da Bacia de Bengala. Além da interpretação sísmica amarrada a alguns poços de controle, o programa de modelagem sedimentar Beicip Franlab Dionisos, foi utilizado para modelar a história de preenchimento da bacia para um período de 5,2 Ma. O nível relativo do nível do mar e a taxa de aporte sedimentar foram os pontos chaves considerados no modelo. Através da utilização dos dados sísmicos, foi possível reconhecer dez quebras de plataformas principais, as quais foram utilizadas no modelo, amarrados aos seus respectivos tempos geológico, provenientes dos dados dos poços do Plioceno ao Holoceno. O resultado do modelo mostrou que a primeira metade modelada pode ser considerada como um sistema deposicional retrogradacional, com algum picos transgressivos. Este sistema muda drasticamente para um sistema progradacional, o qual atuou até o Holoceno. A seção modelada também mostra que no período considerado o total de volume depositado foi em torno de 2,1 x 106 km3, equivalente a 9,41 x 1014 km3/Ma. / The Bengal Basin in Northeast India has a remarkable evolution history directly controled by the Gondwana fragmentation. The Beginning of this basin is considered related to the final break up event, dated as 126 Ma when India finally became separeted from Antarctica and Australia Continents. Since then, the India Continental Plate traveled from the South pole at very fast rate (16 cm/y) reaching the nortern hemisphere and merging with Eurasia Plate. During the travel it passed over a hot spot, located where is today Seychelles Island, resulting in one of the biggest basalt leakage, know as Deccan Trap. In the area where the Bengal Basin was formed during the travel there wasnt any supply of siliciclastics, resulting in the deposition of a very thick section of carbonate platforms from Late Cretaceous to Eocene. After this period, due to the collision with same microplates and the amalgamation with Eurasia Plate a huge siliciclastic supply was introduced in the basin, associated with rising of the Himalayas Mountains. Therefore, the Belgal Basin today has more than 25 km of sediments, collected in its main depocenter. In this dissertation it was applied to the basic concepts of seismostratigraphy in the interpretation of some regional lines. These seismic lines were acquired recently by a special survey program that allowed having good quality data until more than 35 km in the lithosphere (continental and transitional crust). The data permitted to interpret tectonic events such as the presence of Seawards Dipping Reflectors (SDR) in the transitional crust, covered by the Bengal Basin sediments. Besides the seismic interpretation tied to some well data, it was used in the dissertation a Beicip Franlab Software, known as Dionisos, to model and develop a basin fill history. The eustatic relative sea level flutuations and sediment rate of sediment influx are the key points to be considered in the model. Using the seismic data it was possible to recognize ten main platform breakes than were used in the model, tied to a geological time frame provided by the well data interpretation, from Pliocene to Holocene. The output of the model shown that a first half of the considered time predominated a major retrogradational system, with some minor trangression peaks. This changed to a very strong progradational system that is acting until the Holocene. The section modeled also shows a total of sediments deposited in the period considered was about 2,1 x106 km3 equivalent to a 9,41 x 1014 km3/Ma.

Le Cénozoïque est marqué par une instabilité climatique et l’accélération des surrections continentales. Ces phénomènes engendrent une augmentation de la production sédimentaire, transférée par les fleuves vers le domaine marin profond. Les façades nord et ouest de l’océan Indien voient se mettre en place quatre des plus grands systèmes sédimentaires au monde : le Gange-Brahmapoutre, l’Indus, le Zambèze et le système tanzanien. Ce travail vise à comprendre les forçages agissant sur la sédimentation et l’architecture de deux des principaux systèmes turbiditiques de l’océan Indien (système tanzanien et du Gange-Brahmapoutre), pour ensuite les comparer avec leurs plus proches voisins (respectivement le Zambèze et l’Indus). Nos principaux résultats, basés sur une approche multiproxy dans les deux zones, mettent en évidence plusieurs points : (1) l’évolution tectono-sédimentaire de la marge tanzanienne au cours du Cénozoïque a mené au développement d’un système turbiditique majeur et atypique, dont la morphologie moderne atteste de l’importance de l’activité tectonique sur sa construction ; (2) le système du Gange-Brahmapoutre enregistre une activité sédimentaire polyphasée, en lien principalement avec les variations du niveau marin. Ce système est capable d’enregistrer les variations de nombreux forçages, influençant à la fois les bassins versants et le domaine marin. Le fonctionnement sédimentaire et l’architecture des systèmes turbiditiques ont révélé une grande diversité selon le contexte géodynamique et physiographique des façades étudiées. La nécessité d’intégrer l’ensemble des forçages (agissant depuis le bassin versant jusque dans le domaine marin profond) dans l’étude de l’activité sédimentaire d’un système turbiditique apparait essentielle de nos jours. / Cenozoic is marked by climatic instability and accelerating continental uplifts. Increasing sediment yield is generated, buffered and transferred by river to the deep sea. Four of the major turbidite systems in the world are located on the northern and the western margins of the Indian Ocean: the Ganges-Brahmaputra, the Indus, the Zambezi and the Tanzanian systems. This work aims to understand forcings affecting sedimentation and morphology of two main turbidite systems (Tanzanian system and Ganges-Brahmaputra system) and results have been compared with their nearest neighbors (respectively Zambezi and Indus). Based on a multiproxies approach in both area, our main results are as follows: (1) during Cenozoic, tectono-sedimentary evolution of the Tanzania margin led to the development of an atypical turbidite system wherein morphology attest of a strong structural control; (2) the Ganges-Brahmaputra system has a sedimentary activity mainly forced by sea level variations. This turbidite system records variations in many forcings impacting sedimentation from the catchment to the deep sea. Turbidite system activity and architecture revealed a strong variability mainly linked to the geodynamic and physiographic context of each studied margin. It appears necessary to integrate all forcings (affecting both the catchment and the deep sea) in the study and the understanding of sedimentary activity in a turbidite system.