Are Solar Active Regions with Major Flares More Fractal, Multifractal, or Turbulent Than Others?
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/s11207-010-9705-2.pdf
Reference61 articles.
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3. Abramenko, V., Yurchyshyn, V., Wang, H.: 2008, Intermittency in the photosphere and corona above an active region. Astrophys. J. 681, 1669 – 1676. doi: 10.1086/588426 .
4. Abramenko, V.I., Yurchyshyn, V.B., Wang, H., Spirock, T.J., Goode, P.R.: 2002, Scaling behavior of structure functions of the longitudinal magnetic field in active regions on the Sun. Astrophys. J. 577, 487 – 495. doi: 10.1086/342169 .
5. Abramenko, V.I., Yurchyshyn, V.B., Wang, H., Spirock, T.J., Goode, P.R.: 2003, Signature of an avalanche in solar flares as measured by photospheric magnetic fields. Astrophys. J. 597, 1135 – 1144. doi: 10.1086/378492 .
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