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are radio signals that can penetrate through optically thick clouds, radio occultation provides a unique technique to characterize the thermodynamical state within those clouds. This research opportunity
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. Description: This opportunity is closed to applicants who are Senior Fellows (5-years or more past PhD). Clouds, in particular the frozen phase, bring about the largest challenge and uncertainties
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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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clouds, aerosols, and trace gases in the UT/S. In particular, the relationship between atmospheric deep convection, clouds, and water vapor in the tropical upper troposphere and lower stratosphere is a
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. Such mixers will be important for the advancement of astrophysical heterodyne receivers. The main application of these detectors would be in the THz line spectroscopy of the interstellar molecular clouds and
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. Description: The Postdoctoral Fellow will work with a team of world-class collaborators on the JWST Cycle 1 GO Program 2512 (https://www.stsci.edu/jwst/science-execution/program-information.html?id=2512
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due to limitations of model and radiative transfer models (RTM). However, the importance of including radiance data with fields of view (FOVs) affected by clouds and precipitation in a data assimilation
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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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processing to cloud-based computing • Development of highly accessible data bases with in situ computing • Graphics Processing Unit acceleration of scientific data processing Candidates need not have a strong
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Database (Nanograindb; in development). These three databases will enable the study and interpretation of spectral signatures from carbon in the interstellar medium—including molecular clouds, planetary