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National Aeronautics and Space Administration (NASA) | Pasadena, California | United States | about 6 hours ago
electronics for instruments for highly mass-constrained planetary missions. In this project, the fellow should study the pathways to readying a miniature multi-functional instruments with high science value
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National Aeronautics and Space Administration (NASA) | Greenbelt, Maryland | United States | about 6 hours ago
. Description: This opportunity solicits science proposals for the analysis of NASA mission data to study the middle/upper atmospheres and exospheres of planetary bodies in the Solar System. Proposals may focus
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works to translate knowledge into solutions and real-world impact. Learn more about HPH here: https://hph.stanford.edu/ About the Position The Center for Human and Planetary Health is seeking a full-time
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to apply: https://www.jobbnorge.no/en/available-jobs/job/294610/phd-research-fellows-in-geosciences-planetary-or-exoplanetary-sciences-up-to-three-positions Where to apply Website https://www.jobbnorge.no/en
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the Planetary Systems Group (GSP) at the Laboratoire d'Astrophysique de Marseille (UMR7326). The PhD supervisor, Vincent Hue, is a professor at Aix-Marseille Université (CPJ) and a specialist in the atmospheric
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Professor in Planetary Processes. Detailed Position Information The Department of Geological Sciences at The University of Alabama (UA) seeks a tenure-track Assistant Professor in Planetary Processes. We
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current exoplanet-hunting instruments and surveys. A key goal in exoplanet science for the next decade is to improve our understanding of stellar activity, which can masquerade as planetary signals in
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monumental leap in our understanding of planetary systems beyond our own. However, the extreme contrast between the brightness of host stars and the faint light of their orbiting planets poses a formidable
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. Description: ??We develop terahertz instruments working in the 0.1 to 5 THz frequency band for astrophysics, planetary science, and Earth science applications. We provide end-to-end solutions: from device
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to atmospheric density and water vapor content. The radio refractivity profiles evolve in response to the dynamical and thermodynamical processes driving planetary atmospheres. Since the GNSS signals