期刊
SPACE SCIENCE REVIEWS
卷 190, 期 1-4, 页码 103-161出版社
SPRINGER
DOI: 10.1007/s11214-015-0141-3
关键词
Sun: compressible waves; Sun: incompressible waves; Sun: chromosphere; Sun: spicules; Plasma wave heating
资金
- UK Science and Technology Facilities Council (STFC)
- Northumbria University
- Leverhulme Trust (UK)
- Northern Ireland Department for Employment and Learning
- University of Sheffield
- Science and Technology Facilities Council [ST/L002744/1, ST/J001430/1, ST/K004220/1] Funding Source: researchfish
- STFC [ST/L002744/1, ST/K004220/1, ST/J001430/1] Funding Source: UKRI
The chromosphere is a thin layer of the solar atmosphere that bridges the relatively cool photosphere and the intensely heated transition region and corona. Compressible and incompressible waves propagating through the chromosphere can supply significant amounts of energy to the interface region and corona. In recent years an abundance of high-resolution observations from state-of-the-art facilities have provided new and exciting ways of disentangling the characteristics of oscillatory phenomena propagating through the dynamic chromosphere. Coupled with rapid advancements in magnetohydrodynamic wave theory, we are now in an ideal position to thoroughly investigate the role waves play in supplying energy to sustain chromospheric and coronal heating. Here, we review the recent progress made in characterising, categorising and interpreting oscillations manifesting in the solar chromosphere, with an impetus placed on their intrinsic energetics.
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