J. D. Haiducek

TL;DR: In this paper, a two-way coupled kinetic-fluid model was used to simulate the interaction between Jupiter's magnetospheric plasma and Ganymede's magnetosphere.

TL;DR: In this paper, the formation and evolution of plasma interaction regions at the comet 67P/Churyumov-Gerasimenko (67P/CG) were observed.

TL;DR: In this paper, the authors simulated the entire month of January 2005 using the Space Weather Modeling Framework (SWMF) with observed solar wind data as input, and evaluated the model's accuracy in predicting Kp, SYM-H, AL, and cross-polar cap potential (CPCP).

TL;DR: Zdanov et al. as discussed by the authors used coupled computational fluid dynamics (CFD) and optics solvers, which were three-dimensional and time-dependent The CFD code used a cell-centered, conservative, finite-volume discretization of the integral form of the Navier-Stokes equations It included thermal energy transport and mass conservation, which accounted for chemical reactions and state kinetics.

TL;DR: The SHIELDS framework as discussed by the authors was developed to understand the dynamics of the surface charging environment (SCE), the hot (keV) electrons representing the source and seed populations for the radiation belts, on both macro-and micro-scale.