How to Reach Superequipartition Field Strengths in Solar Magnetic Flux Tubes
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/s11207-007-9072-9.pdf
Reference35 articles.
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3. Bellot-Rubio, L.R., Rodríguez-Hidalgo, I., Collados, M., Khomenko, E., Ruiz-Cobo, B.: 2001, Observation of convective collapse and upward-moving shocks in the quiet Sun. Astrophys. J. 560, 1010 – 1019.
4. Brandenburg, A.: 2005, The case for a distributed solar dynamo shaped by near-surface shear. Astrophys. J. 625, 539 – 547.
5. Caligari, P., Moreno-Insertis, F., Schüssler, M.: 1995, Emerging flux tubes in the solar convection zone I. Asymmetry, tilt, and emergence latitude. Astrophys. J. 441, 886 – 902.
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