93 parallel-and-distributed-computing-phd Postdoctoral positions at The Ohio State University
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University studying microbial ecology of glacier and permafrost environments. The Post Doctoral Scholar will embark on a program of independent research with the primary goal of determining how microorganisms
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for submission to peer-reviewed journals; and mentoring undergraduate and graduate students. Other responsibilities include field research program and conference presentations. Qualifications: PhD in glaciology
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. The Post Doctoral Scholar will embark on a program of independent research with the primary goal of determining how computational and theoretical methods can provide thermodynamic design principles
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instrumentation. It involves supervising the research of graduate students and REU’s, conceiving, composing, writing and editing research proposals, scientific papers and research reports. Required Education: PhD
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background in analyzing large astronomical datasets is essential, particularly in characterizing non-isotropic distributions and spatial-kinematic properties using Gaia and/or DESI data. Proficiency in
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activities, including the submission of new grant applications, related to their work. Required Education: PhD in Engineering Biomechanics, Engineering Mechanics or related field Required Experience: Computer
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will also be considered. Strong background in analyzing large astronomical datasets is essential, particularly in characterizing non-isotropic distributions and spatial-kinematic properties using Gaia
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on ongoing and new research projects. Participate in writing research papers and presenting results at seminars, workshops, and conferences. Qualifications Required: PhD in Computer Science or Math Strong
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engineering related research, makes and records observations and measurements, collects and compiles data for computer input and analysis, perform literature search on related topics, and operates and maintains
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that govern time-dependent spectral energy distributions of black hole accretion disks, applying these models to X-ray and multi-wavelength data to extract empirical constraints on accretion flow physics, and