Thesis (S.M.)--Joint Program in Oceanography (Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences and the Woods Hole Oceanographic Institution), 2001. / Includes bibliographical references (leaves 44-48). / Megamullions in slow-spreading oceanic crust are characterized by smooth "turtle-back" morphology and are interpreted to be rotated footwalls of long-lived detachment faults. Megamullions have been analyzed in preliminary studies, but many questions remain about structural and tectonic details of their formation, in particular how the hanging wall develops in conjugate crust on the opposing side of the rift axis. This study compares the structure of an off-axis megamullion complex and its conjugate hanging wall crust on the Mid-Atlantic Ridge near 27 0N. Two megamullion complexes, an older (Ml) and younger (M2), formed successively on the west side of the rift axis in approximately the same location within one spreading segment. Megamullion M1 formed while the spreading segment had only one inside comer on the west flank, and megamullion M2 formed after the segment developed double inside corners west of the axis and double outside corners east of the axis. The older megamullion formed between -22.3 and -20.4 Ma, and the younger megamullion formed between -20.6 and -18.3 Ma; they are presently -200-300 km off-axis. Reconstruction poles of plate rotation were derived and plate reconstructions were made for periods prior to initiation of the megamullion complex (anomaly 6Ar, -22.6 Ma), after the termination of megamullion Ml and during the development of megamullion M2 (anomaly 5E, -19 9 Ma), and shortly following the termination of megamullion M2 (anomaly 5C, -17.6 Ma). These reconstructions were used to compare morphological and geophysical features of both flanks at each stage of the megamullions' development. Megamullion Ml's breakaway occurred at -22.3 Ma and slip along this detachment fault continued and propagated northward at -20.6 Ma to form the northern portion of M2. The exhumed footwall of megamullion M1 has weak spreading-parallel lineations interpreted as mullion structures on its surface, and it forms an elevated plateau between the enclosing segment boundaries (non-transform discontinuities). There was an expansion southward of the detachment fault forming megamullion M2 at -20.1 Ma. It either cut a new detachment fault through megamullion Ml, stranding a piece of megamullion Ml on the conjugate side (east flank), or it linked into the active detachment fault that was forming megamullion M1 or propagated into its hanging wall. The expanded detachment of megamullion M2 and the termination of megamullion M1 occurred during a time when the enclosing spreading segment roughly doubled in length and formed two inside corners. Megamullion M2 developed prominent, high-amplitude (-600 m) mullion structures that parallel the spreading direction for more than 20 km at each inside corner. Its detachment fault was abandoned - 18.6 Ma in the south and ~18.3 Ma in the north ... / by Amy R. McKnight. / S.M.

Thesis. 1976. M.S.--Massachusetts Institute of Technology. Dept. of Earth and Planetary Sciences. / Microfiche copy available in Archives and Science. / Bibliography: leaves 51-58. / by Jeremy D. Duschenes. / M.S.

Thesis (Ph.D.)--Massachusetts Institute of Technology, Dept. of Earth and Planetary Sciences, 1980. / Microfiche copy available in Archives and Science. / Vita. / Bibliography : leaves 206-213. / by John Shai-Fu Shih. / Ph.D.

Thesis. 1978. Ph.D.--Massachusetts Institute of Technology. Dept. of Earth and Planetary Science. / Microfiche copy available in Archives and Science. / Vita. / Includes bibliographies. / by Robert Sherman Detrick, Jr. / Ph.D.

Thesis (Ph.D.)--Massachusetts Institute of Technology, Dept. of Earth and Planetary Sciences, 1979. / Microfiche copy available in Archives and Science. / Vita. / Includes bibliographies. / by Christopher Robert Tapscott. / Ph.D.

Thesis. 1977. Ph.D.--Massachusetts Institute of Technology. Dept. of Earth and Planetary Sciences. / Microfiche copy available in Archives and Science. / Vita. / Bibliography : leaves 223-233. / Ph.D.

Ce mémoire de thèse est consacré à la mise en place d'un système opto-électronique générique basé sur une liaison toute optique bidirectionnelle de 10km. L'architecture étudiée et développée est dédiée à l'extension d'un observatoire câblé de fond de mer afin d'atteindre de nouvelles zones d'exploration. Les travaux de recherche rapportés dans ce manuscrit présentent la réalisation d'un démonstrateur, qui permet la récupération de données, issues d'un instrument connecté à un module opto-alimenté, via une seule fibre optique où transitent simultanément deux voies de données en bande C et la puissance optique d'alimentation (à 1480nm) égale à 33dBm permettant de récupérer 180mW électrique sur le module opto-alimenté.Le contexte de cette thèse de doctorat est présenté au travers d'un état de l'art sur les moyens utilisés pour l'observation des océans et sur les systèmes électroniques à faible consommation. Après un rappel des caractéristiques essentielles de l'architecture de la liaison optique préalablement établie, nous nous concentrons sur la structure opto-électronique qui a pour but d’assurer la communication entre l’observatoire et l’instrument déporté de l’extension. La définition du cahier des charges a abouti au choix du capteur (hydrophone), du débit des données (5Mbit/s) et du protocole de communication (SPI 3-fils) utilisé entre les deux modules opto-électroniques, chacun à une extrémité de la fibre optique. L'effort a été porté sur la conception d'un module opto-alimenté faible consommation (66mW) où s'intègre l'instrument. Tout au long de ce document, les choix technologiques retenus lors de la conception des deux modules opto-électroniques sont argumentés. Le banc d'essai du démonstrateur a permis de valider la conception de cette extension et d'évaluer la qualité de la transmission des données (BER inférieur à 10-6). Le fonctionnement d'un premier prototype destiné à être marinisé a été présenté au travers de la détection et de la transmission de signaux acoustiques générés en bassin d'essai. De manière à rendre le système encore plus générique, une solution alternative à base d'un FPGA, permettant l'utilisation d'une interface SPI 4-fils sans modifier la liaison optique a été présentée et validée. / This PhD thesis is devoted to the design of an opto-electrical and generic system which uses a 10km long all-optical and bidirectional link. The studied and developed system is dedicated to extend a current cabled seafloor observatory, in order to reach new exploration areas. The research work described in this thesis presents the development and the realization of a demonstrator. This later collects data from an instrument connected to its optically powered unit. The optical power supply (33dBm at 1480nm), which provides up to 180mW electrical for the optically powered unit, and the optical data in C band, are transmitted simultaneously through the same single optical fiber.The thesis context is first presented through an overview of ocean observation systems and low consumption electronic devices. After a brief review on the main characteristics of the optical architecture, we focused on the opto-electrical structure which permits the communication between the observatory and the remote instrument. The desired requirements have led us to the choice of the sensor (hydrophone), the data bit rate (5Mbit/s) and the communication protocol (SPI 3-Wire) used between both opto-electrical units, each one located at the both ends of the optical link. A special attention was devoted to the conception of the optically powered which must be low power consumption (66mW). All along this document, technical choices involved in the realization of both opto-electrical units are presented. We could evaluate the performance of the data transmission (BER less than 10-6) by using a demonstrator's test bench. Then, a first prototype designed for the ocean environment was presented through experimental measurements. Those tests were conducted in a test pool and have consisted in the detection of acoustic signals. In order to increase the range of compatible instruments, an alternative solution based on a FPGA was described and approved. This new design allows the SPI 4-Wire to be employed without any change of the current optical architecture.

Thesis (doctoral)--Universität Bremen, 2005. / Includes bibliographical references (p. 113-125).

The Hess Deep Rift in the East Pacific Rise is a mid-ocean ridge spreading center that produces melts which exhibit geochemical characteristics of evolved MORB. Using basaltic glass samples collected from multiple dive cruises that explored Hess Deep geology, volatile and chemical data were collected at USF using FTIR and EMPA, respectively. In addition, a data suite of samples of glass from Hess Deep were compiled from the EarthChem database. The intention was to use the data suite and models to compare the Hess Deep regime to analog models for mid-ocean ridge crystallization regimes and tectonic structures. The USF and EarthChem samples were then compared to various crystallization models generated in Petrolog3 (Danyushevsky and Plechov, 2011) and COMAGMAT (Ariskin and Barmina, 2004). The starting compositions using depleted, normal, and enriched MORB (Gale et al, 2013) were modeled at depths reflecting an upper and lower melt lens along the rift axis. The volatile components of the USF samples were compared to models for water and carbon dioxide behavior in basalt made using VolatileCalc (Newman and Lowenstern, 2002). Based on the comparison of the samples to the forward modeling in Petrolog3, it appears that the geochemical behavior of major and trace elements most closely resembles that of small amounts of fractional crystallization and re-assimilation of accessory minerals. The VolatileCalc models suggest that the USF samples most likely followed a degassing pathway at depths corresponding to the shallow melt lens. When considering the analog models for ophiolite sequences and melt flow beneath a fast-spreading ridge, it appears that the melt regime at Hess Deep deviates from both standing theories. Instead the most likely mechanisms are shallow crystallization, at depths equal to or less than an upper melt lens, and shallow dynamic degassing.

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