From Theoretical Foundation to Invaluable Research Tool: Modern Hybrid Simulations
D. Krauss-Varban
Abstract
In many plasmas, in particular in space science, protons govern much of the essential physics. Minority ions, suprathermal tails, and electrons at times account for additional details. However, electron effects usually appear on much smaller spatial and temporal scales. For more than two decades, scientists have refined computational models that concentrate on the dominating and larger-scale ion kinetic physics, while treating the much lighter electrons as a charge-neutralizing fluid. These physics-based, algorithmic model descriptions are called hybrid codes, which have established an invaluable position for themselves - clearly distinct from MHD calculations, but simpler and much more efficient than full-particle simulations. Here, the foundation and numerical details of hybrid codes are reviewed, and differences between existing algorithms are elucidated.
Create a lesson
Related papers
Statistical Models of Ionospheric Variability and Irregularities in the Topside Ionosphere Based on the Swarm Satellite Data
Daria Kotova, Alan Wood, Eelco Doornbos et al.
A quiet STEVE disturbs navigation satellites' signals in the Antarctic
Daria Kotova, Luca Spogli, Yaqi Jin et al.
Empirical Relationship for Geomagnetically Induced Currents (GIC) and Solar Wind Conditions
Dean Thomas, Lucy A. Wilkerson, Robert S. Weigel et al.
Comprehensive solar eruption analyses enabled by the tools of the SOLER project
Nina Dresing, Jan Gieseler, Markus Baumgartner-Steinleitner et al.
Evolution of lunar wake potentials: structure, energy conversion, and their imprints on velocity distributions
Xin An, Vassilis Angelopoulos, Jasper S. Halekas et al.
In-situ measurements of space plasma: recent progress and future challenges
Daniel Verscharen