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dc.contributor.advisorBenjamin P. Weiss.en_US
dc.contributor.authorSchnepf, Neesha Regmien_US
dc.contributor.otherMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences.en_US
dc.date.accessioned2015-09-17T19:03:56Z
dc.date.available2015-09-17T19:03:56Z
dc.date.copyright2015en_US
dc.date.issued2015en_US
dc.identifier.urihttp://hdl.handle.net/1721.1/98673
dc.descriptionThesis: S.M., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, 2015.en_US
dc.descriptionCataloged from PDF version of thesis.en_US
dc.descriptionIncludes bibliographical references.en_US
dc.description.abstractThe 20 th century brought many breakthroughs in our understanding of Earth, but there are still many outstanding geophysical questions. Deep electromagnetic studies provide information on electrical conductivity from the near-surface to deep within the mantle (~1600 km) complementing seismic work aiming understand the composition, structure and dynamics of the mantle. Electromagnetic induction studies utilize the skin depth concept which relates the period of a source electromagnetic field and the conductivity of the penetrated material with the maximum depth the field can penetrate. Traditional satellite-based induction studies use signals of magnetospheric origin and considered a period range between a few days and a few months. These traditional studies are mostly sensitive to deep conducting structures because of the inductive coupling between primary and induced sources. In contrast, galvanic coupling from the oceanic tidal signal allows for studying less conductive, shallower structures by also using shorter periods. A few studies convincingly demonstrated that the magnetic fields induced by the lunar semidiurnal ocean tide can be identified in satellite observations. This result encourages using tidal satellite magnetic data to constrain subsurface electrical conductivity in oceanic regions. We perform global 3- D electromagnetic numerical simulations to investigate the sensitivity of the ocean's tidal signals magnetic amplitudes to conductivity distributions at different depths. The results of our sensitivity analysis suggest it will be promising to use oceanic signals detected at satellite altitude for probing lithospheric and upper mantle conductivity. Our simulations also suggest that seafloor electric and magnetic field data may provide complementary details to better constrain lithospheric conductivity.en_US
dc.description.statementofresponsibilityby Neesha Regmi Schnepf.en_US
dc.format.extent69 pagesen_US
dc.language.isoengen_US
dc.publisherMassachusetts Institute of Technologyen_US
dc.rightsM.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission.en_US
dc.rights.urihttp://dspace.mit.edu/handle/1721.1/7582en_US
dc.subjectEarth, Atmospheric, and Planetary Sciences.en_US
dc.titleCan we probe the conductivity of the lithosphere and upper mantle using satellite ocean tidal magnetic signals?en_US
dc.title.alternativeSensing the upper mantle and lithosphere using ocean tidal magnetic field satellite measurementen_US
dc.typeThesisen_US
dc.description.degreeS.M.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
dc.identifier.oclc920682504en_US


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