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with data-based models and numerical dynamo simulations. The successful candidate will contribute to studies of time-averaged geomagnetic field morphologies and core dynamics during transitional events
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the chemical composition and evolution of the disc, and will perform numerical simulations of planet formation to constrain the formation of terrestrial planets in the solar system. The candidate is further
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Alfred-Wegener-Institut Helmholtz-Zentrum für Polar- und Meeresforschung | Bremerhaven, Bremen | Germany | about 1 month ago
analyzing numerical simulations of the Arctic Ocean with explicit tidal forcing to study the role of tides for Arctic Ocean dynamics and sea ice and vice versa Estimating the numerical internal tide
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short time scale, such as a few seconds to ten minutes, and ionospheric parameter estimation Validate the results from VGOS with GNSS, numerical weather model, and water vapor radiometer Collaborative
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Helmholtz-Zentrum Dresden-Rossendorf - HZDR - Helmholtz Association | Dresden, Sachsen | Germany | about 1 month ago
balance with the possibility of part-time employment, mobile working and flexible working hours # Numerous company health management offerings # Employee discounts with well-known providers via the platform
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Helmholtz-Zentrum Dresden-Rossendorf - HZDR - Helmholtz Association | Dresden, Sachsen | Germany | 27 days ago
, mobile working and flexible working hours # Numerous company health management offerings # Employee discounts with well-known providers via the platform Corporate Benefits # An employer subsidy
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framework; Validate the coupled model using published and newly gathered observational data; Conduct numerical experiments to understand responses to changing lightscapes and to unravel future pathways across
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; Couple the model to a 1D physical model (GOTM) through the FABM framework; Validate the coupled model using published and newly gathered observational data; Conduct numerical experiments to understand
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Electrodynamics General Circulation Model (TIE-GCM) is a global 3D numerical model that simulates the coupled ionosphere-thermosphere system from ∼97 to ∼600 km height. It self-consistently solves the fully coupled
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Your Job: This project uses numerical simulations to determine the relative importance of the presence of interstellar objects (ISOs) in the interstellar medium. Specifically, the various formation