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- W1937245718 endingPage "448" @default.
- W1937245718 startingPage "431" @default.
- W1937245718 abstract "Within the last decade, due to significant improvements in the spatial and temporal resolution of chromospheric data, magnetohydrodynamic (MHD) wave studies in this fascinating region of the Sun's atmosphere have risen to the forefront of solar physics research. In this review we begin by reviewing the challenges and debates that have manifested in relation to MHD wave mode identification in fine-scale chromospheric magnetic structures, including spicules, fibrils and mottles. Next we go on to discuss how the process of accurately identifying MHD wave modes also has a crucial role to play in estimating their wave energy flux. This is of cardinal importance for estimating what the possible contribution of MHD waves is to solar atmospheric heating. Finally, we detail how such advances in chromospheric MHD wave studies have also allowed us, for the first time, to implement cutting-edge magnetoseismological techniques that provide new insight into the sub-resolution plasma structuring of the lower solar atmosphere." @default.
- W1937245718 created "2016-06-24" @default.
- W1937245718 creator A5025928183 @default.
- W1937245718 creator A5046122084 @default.
- W1937245718 date "2016-02-12" @default.
- W1937245718 modified "2023-09-26" @default.
- W1937245718 title "MHD Wave Modes Resolved in Fine-Scale Chromospheric Magnetic Structures" @default.
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- W1937245718 doi "https://doi.org/10.1002/9781119055006.ch25" @default.
- W1937245718 hasPublicationYear "2016" @default.