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- W2617852024 startingPage "012014" @default.
- W2617852024 abstract "The solar eruptions and interacting solar wind streams are key drivers of geomagnetic storms and various related space weather disturbances that may have hazardous effects on the space-borne and ground-based technological systems as well as on human health. Coronal mass ejections (CMEs) and their interplanetary counterparts, interplanetary CMEs (ICMEs), belong to the strongest disturbances and therefore are of great importance for the space weather predictions. In this paper we show a few examples of how adaptive mesh refinement makes it possible to resolve the complex CME structure and its evolution in time while a CME propagates from the inner boundary to Earth. Simulations are performed with the Multi-Scale Fluid-Kinetic Simulation Suite (MS-FLUKSS)." @default.
- W2617852024 created "2017-06-05" @default.
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- W2617852024 date "2017-05-30" @default.
- W2617852024 modified "2023-09-23" @default.
- W2617852024 title "Modeling Coronal Mass Ejections with the Multi-Scale Fluid-Kinetic Simulation Suite" @default.
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- W2617852024 doi "https://doi.org/10.1088/1742-6596/837/1/012014" @default.
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