140 evolution "https:" "https:" "https:" "https:" "https:" "https:" "U.S" "U.S" "St" "St" uni jobs at Zintellect in United States
Sort by
Refine Your Search
-
Countries can be found at: https://www.nasa.gov/oiir/export-control . Eligibility is currently open to: U.S. Citizens; U.S. Lawful Permanent Residents (LPR); Foreign Nationals eligible for an Exchange Visitor
-
. 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
-
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
-
. 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
-
the Research and Development Directorate of DTRA, Test and Assessment Department. For more information about the DTRA, please visit https://www.dtra.mil/ . About ORISE This program, administered by Oak Ridge
-
about this opportunity? Please email npp@orau.org Point of Contact Mikeala Eligibility Requirements Citizenship: U.S. Citizen Only Degree: Doctoral Degree. ORAU Pathfinder Whether you are just starting
-
, active geologic processes, vegetation traits, and algal biomass using hyperspectral imagery in the visible and shortwave infrared and multi- or hyperspectral imagery in the thermal IR (https
-
at: https://www.nasa.gov/oiir/export-control . Eligibility is currently open to: U.S. Citizens; U.S. Lawful Permanent Residents (LPR); Foreign Nationals eligible for an Exchange Visitor J-1 visa status; and
-
at: https://www.nasa.gov/oiir/export-control . Eligibility is currently open to: U.S. Citizens; U.S. Lawful Permanent Residents (LPR); Foreign Nationals eligible for an Exchange Visitor J-1 visa status; and
-
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