206 evolution-"https:" "https:" "https:" "UCL" "UCL" "UCL" "UCL" positions at Zintellect
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. Description: The balance of infall and outflow of circumgalactic gas determines the long-term evolution of a galaxy, so understanding how gas gets into and out of galaxies is essential to understanding our
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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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, California Field of Science: Technology Development Advisors: Goutam Chattopadhyay Goutam.Chattopadhyay@jpl.nasa.gov 818-393-7779 Applications with citizens from Designated Countries will not be accepted
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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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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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) 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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SPHEREx satellite. Likewise, data analysis on the dust lifecycle, dust composition in nearby galaxies, ice formation and evolution, Zodiacal dust, and the connections between dust and gas are possible with
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. Description: Multidisciplinary studies are ongoing that involve the development and field testing of drilling and sample handling systems and automation technologies to operate these systems. NASA Ames
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include remote sensing algorithm development, modeling studies, data fusion, sensor development, and/or snow satellite mission concept studies. Participation in the design and execution of field campaigns
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can be measured to understand spot coverage and spot evolution and simultaneous observations of flares from the X-ray to radio can lead to deep insight into flare emission mechanisms, flare energy