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- W2028262011 abstract "[1] The importance of specifying and predicting the state of the Earth's space environment, i.e., space weather, has recently been increasingly realized, as dynamic activities of the Sun, solar wind, magnetosphere, and ionosphere can influence modern technology systems and even endanger human life. It is also widely recognized that numerical simulations driven by integrated ground-based and satellite observations are a powerful tool for quantitatively understanding the complex Sun-Earth system, and they are a vital means for predicting space weather. [2] It is required, however, that a physical model of solar-terrestrial phenomena be constructed as a basis of space weather predictions. The model must deal with the key processes spanning from flares and coronal mass ejections on the Sun to geomagnetic storms and their effects in the upper atmosphere of Earth. To reach the goal effectively, it is acute to ask a number of fundamental questions such as, What is the triggering condition of solar flares and coronal mass ejections (CMEs)? What mechanism generates fast reconnection and leads to particle acceleration? Why particular solar flares cause superstorms on Earth? Working out these basic questions is probably equivalent to understanding multiscale coupling of various physical processes occurring in the Sun-Earth system on different scales. It is indispensable that the communications among different fields, especially between the solar and geophysical communities, be enhanced more systematically. [3] This special section results primarily from the CAWSES International Workshop on Space Weather Modeling (CSWM), which was held on 14–17 November 2006 in Yokohama, Japan, but includes several papers that were not presented at the Workshop. It is hoped that this section will provide a timely forum for discussing all aspects of space weather modeling research, aiming to summarize the current status and future prospects of this rapidly growing field. It contains original research papers as well as topical review papers on the advanced modeling of solar and heliospheric magnetic field; solar flares, CMEs, and filament eruption; solar wind; geomagnetic storms; and radiation belts." @default.
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- W2028262011 date "2008-02-05" @default.
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- W2028262011 title "Introduction to special section on Space weather modeling: Status and prospects" @default.
- W2028262011 doi "https://doi.org/10.1029/2007ja012972" @default.
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