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- W3098578184 abstract "The physical processes, which drive powerful solar eruptions, play an important role in our understanding of the Sun-Earth connection. In this Special Issue, we firstly discuss how magnetic fields emerge from the solar interior to the solar surface, to build up active regions, which commonly host large-scale coronal disturbances, such as coronal mass ejections (CMEs). Then, we discuss the physical processes associated with the driving and triggering of these eruptions, the propagation of the large-scale magnetic disturbances through interplanetary space and the interaction of CMEs with Earth's magnetic field. The acceleration mechanisms for the solar energetic particles related to explosive phenomena (e.g. flares and/or CMEs) in the solar corona are also discussed. The main aim of this Issue, therefore, is to encapsulate the present state-of-the-art in research related to the genesis of solar eruptions and their space-weather implications. This article is part of the theme issue 'Solar eruptions and their space weather impact'." @default.
- W3098578184 created "2020-11-23" @default.
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- W3098578184 date "2019-05-13" @default.
- W3098578184 modified "2023-09-24" @default.
- W3098578184 title "Introduction to the physics of solar eruptions and their space weather impact" @default.
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- W3098578184 doi "https://doi.org/10.1098/rsta.2019.0152" @default.
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