The HYPERS code was developed in the early 2010's by Yuri Omelchenko as a general-purpose hybrid code for modeling multiscale fusion and space plasmas with significant kinetic ion effects. At the ...
The HESPERIA Relativistic Electron Alert System for Exploration (RE-leASE) model uses the fact that near relativistic electrons (1 MeV electrons travel at 95% of the speed of light) travel faster than ...
Models: Wang-Sheeley-Arge version WSA-1.6 (N. Arge) corona, ENLIL version ENLIL-ccmc-2.6 (D. Odstrcil) heliosphere. The magnetic footpoint of Earth is displayed for the 10 latest days of the solar ...
The OVATION Prime model was developed using energetic particle measurements from the polarorbiting Defense Meteorological Satellite Program (DMSP) satellites and considers four types of aurorae: two ...
KASI Geomagnetic Storm Forecast Model is an empirical model to forecast not only the geomagnetic storm strength in Dst index, but also its possibility based on initially observed parameters of coronal ...
The Tsyganenko models are semi-empirical best-fit representations for the magnetic field, based on a large number of satellite observations (IMP, HEOS, ISEE, POLAR, Geotail, GOES, etc). The models ...
NASA's Community Coordinated Modeling Center (CCMC) provides free access to space weather models, simulation runs-on-request, real-time space weather predictions, visualization tools, and model ...
CORHEL-CME, developed by Predictive Science Inc., is a novel MHD modeling framework specifically designed to be used by non-experts. It consists of a collection of tools and simulation codes that are ...
4 Day Advanced Predictions and Satellite observations WSA SWPC_REALTIME Oct 30 10:00 Solar Wind Speed (km/s) SWPC_REALTIME is collocated with L1 and is a composite dataset of SOLAR-1, IMAP, and ACE.
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