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APPLICATION INSTRUCTIONS: CURRENT PENN STATE EMPLOYEE (faculty, staff, technical service, or student), please login to Workday to complete the internal application process . Please do not apply
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of human serum, plasma, urine or other clinical samples RT-qPCR, RNA sequencing or other molecular/omics techniques bioinformatics, biostatistics or integration of molecular and clinical data Hands
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searching for a computational postdoctoral research associate. The project is associated with atomistic plasma-surface interaction simulations, employing machine learned interatomic potentials (MLIPs
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linkage with incubation and start-up ecosystems. About ACER: The center has been recently created to address enduring process challenges in Chemistry and Engineering disciplines and create an environment
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Max Planck Institute of Molecular Physiology, Dortmund | Dortmund, Nordrhein Westfalen | Germany | about 1 month ago
areas: plasma physics, cryogenics, light and electron microscopy, microfabrication, image processing software development, cryogenic electron tomography Proven research track record (publications
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Austrian Academy of Sciences, The Marietta Blau Institute for Particle Physics (MBI) | Austria | 2 months ago
particles (single particle and non-neutral plasma regimes). Positron and positronium physics (positron beams, detection etc.). Ion physics (production, mass spectrometry). Proven track-record of both
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diversity of platforms and building blocks. The foundry model is now becoming established where Process Design Kits (PDKs) allow fabless designers to create their own chips with custom functionality. While
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technologies for remote detection. Specifically, this position involves research on generation of widely tunable GHz-THz femtosecond pulse bursts to optimize laser-matter coupling, plasma generation, and
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National Aeronautics and Space Administration (NASA) | Huntsville, Alabama | United States | 15 days ago
hotter plasma at greater heights on the Earth-facing solar disk than is currently accessible. Achieving this capability, however, requires significant advances in EUV coatings, detector technology
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; plasmas encountered in planetary magnetospheres; the solar wind and artificially generated charges and fields on spacecraft; micro-meteoroids and non trackable debris; planetary and lunar dust; and