Alfvén Waves in the Solar Atmosphere: From Theory to Observations
Alfvén waves are considered to be viable transporters of the non-thermal energy required to heat the Sun’s quiescent atmosphere. An abundance of recent observations, from state-of-the-art facilities, have reported the existence of Alfvén waves in a range of chromospheric and coronal structures. Here...
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| Veröffentlicht in: | Space science reviews 2013-06, Vol.175 (1-4), p.1-27 |
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| container_title | Space science reviews |
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| creator | Mathioudakis, M. Jess, D. B. Erdélyi, R. |
| description | Alfvén waves are considered to be viable transporters of the non-thermal energy required to heat the Sun’s quiescent atmosphere. An abundance of recent observations, from state-of-the-art facilities, have reported the existence of Alfvén waves in a range of chromospheric and coronal structures. Here, we review the progress made in disentangling the characteristics of transverse kink and torsional linear magnetohydrodynamic (MHD) waves. We outline the simple, yet powerful theory describing their basic properties in (non-)uniform magnetic structures, which closely resemble the building blocks of the real solar atmosphere. |
| doi_str_mv | 10.1007/s11214-012-9944-7 |
| format | Article |
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| subjects | Aerospace Technology and Astronautics Astrophysics and Astroparticles Atmosphere Corona Fluid mechanics Physics Physics and Astronomy Planetology Propagation Solar physics Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Sun Thermal energy |
| title | Alfvén Waves in the Solar Atmosphere: From Theory to Observations |
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