280 developer-"https:" "https:" "https:" "Lawrence Berkeley National Laboratory Physics" positions at Zintellect
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models to be developed for cosmological analyses. At JPL, there are opportunities to pursue one or more of these facets of dust astrophysics, particularly as they relate to past, present, and future NASA
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. Current research focuses primarily on the development of large-format arrays of sensitive bolometers using superconducting transition edge sensors. We also have investigated single pixel optimization
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. Description: Our research focuses on understanding basic processes which occur in solar and stellar flares through analyzing data, development of theory, and computational studies. Specifically, we are seeking
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for determination of errors in path delay modeling; (2) understanding the origin of these errors; and (3) working to develop methodologies for mitigation of these wet-delay errors. In addition to deterministic
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polarimetric observations are developed. Specifically, this research utilizes a wide range of radiative measurements across the shortwave solar spectrum to derive properties of atmospheric particulate, including
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available for projects related to the development and exploitation of cosmological numerical simulations and mock galaxy catalogs for weak lensing and galaxy clustering. These efforts will feed directly into
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. Description: Our objective is to develop techniques to manufacture x-ray telescopes with five characteristics: high angular resolution, high throughput, light weight, low cost, and efficient production. Two
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capbilities include testing on high altitude balloons. For the past year we have hosted the award-winning Stanford-Brown iGEM team, whose wikis will give additional background in lab activities. http://2011
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) Structure formation of the Universe and evolution of clusters of galaxies; (2) Circulation history of baryonic matter in the Universe; (3) Transport and circulation of energy in the Universe; (4) New science
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can enable low-cost and long-lasting planetary exploration missions to hot planets. Our research objective is to develop a sensor technology platform that is temperature and radiation tolerant using