Saturation level of Alfvén waves driven by Kelvin–Helmholtz instability
Author:
Publisher
Springer Science and Business Media LLC
Subject
Multidisciplinary
Link
http://link.springer.com/content/pdf/10.1007/s11434-014-0421-4.pdf
Reference62 articles.
1. Alfvén H (1942) Existence of electromagnetic-hydrodynamic waves. Nature 150:405–406
2. Bostick WH, Levine MA (1952) Experimental demonstration in the laboratory of the existence of magneto-hydrodynamic waves in ionized helium. Phys Rev 87:671–671
3. De Pontieu B, McIntosh SW, Carlsson M et al (2007) Chromospheric Alfvénic waves strong enough to power the solar wind. Science 318:1574–1577
4. McIntosh SW, de Pontieu B, Carlsson M et al (2011) Alfvénic waves with sufficient energy to power the quiet solar corona and fast solar wind. Nature 475:477–480
5. Tomczyk S, McIntosh SW, Keil SL et al (2007) Alfvén waves in the solar corona. Science 317:1192–1196
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