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• W1502016772 abstract "There is an increasing need to develop physics-based, high performance models of the Sun-Earth system - from the solar surface to the Earth's upper atmosphere - which can operate faster than real time and which can provide reliable predictions of the near Earth space environment based upon solar observations and upstream solar wind measurements. Taking advantage of the advent of massively parallel computers, sophisticated solution-adaptive techniques, and recent fundamental advances in basic numerical methods we have developed a high performance, multiscale MHD code capable of resolving many of the critical processes in the Sun-Earth system which range over more than 9 orders of magnitude. We report on the first comprehensive numerical simulation of a synthetic space weather event, starting with the generation of a CME and subsequently following this transient solar wind disturbance as it evolves into a magnetic cloud and travels through interplanetary space towards Earth where its interaction with the terrestrial magnetosphere-ionosphere system is also predicted as part of the simulation." @default.
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• W1502016772 date "2013-03-19" @default.
• W1502016772 modified "2023-10-14" @default.
• W1502016772 title "From Sun to Earth: Multiscale MHD Simulations of Space Weather" @default.
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• W1502016772 doi "https://doi.org/10.1029/gm125p0169" @default.
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