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of solar system history, recording planetary differentiation, impact flux, and volatile evolution more completely and more clearly than any other planetary body. Asteroids are fascinating worlds ranging from
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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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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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their evolution through time. To that end we are seeking an NPP applicant to develop methodologies to invert for time-evolving basal friction from massive volumes of surface flow observations
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the galaxy from their sources to the Earth. A developed Monte Carlo computer code is used to study the acceleration process by plasma shocks, while mathematical models have been designed to describe how
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Dust Grains by generating laboratory experimental and quantum computational data, and developing associated tools. These will be provided to the scientific community via three complementary databases
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to support investigations focused on short and long-term evolution of cloud/aerosol properties, dynamical flows, and transient phenomena. Studies of specific atmospheric features, such as Jupiter‘ Great Red
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surface, aerosols, clouds, and climate change. In-house capabilities include design and development of novel airborne instruments for aerosol, cloud and trace gases systems. For the past year, we hosted a
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retrieval algorithm development with focus on using the polarimetric signals, the new FIR or sub-mm bands, and/or the ML/AI approach; (3) ML/AI application on system/pattern tracking on satellite images
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development work could focus on moving towards hyper-resolution land surface representations, assimilation or observations, or downscaling and improvement of forcing data. Location: Jet Propulsion Laboratory