The Origin, Early Evolution and Predictability of Solar Eruptions
Author:
Green Lucie M.ORCID,
Török Tibor,
Vršnak Bojan,
Manchester Ward,
Veronig Astrid
Publisher
Springer Netherlands
Reference391 articles.
1. W.P. Abbett, The magnetic connection between the convection zone and corona in the quiet sun. Astrophys. J. 665, 1469–1488 (2007).
https://doi.org/10.1086/519788
2. W.P. Abbett, G.H. Fisher, Y. Fan, The effects of rotation on the evolution of rising omega loops in a stratified model convection zone. Astrophys. J. 546, 1194–1203 (2001).
https://doi.org/10.1086/318320
.
arXiv:astro-ph/0008501
3. J.J. Aly, On some properties of force-free magnetic fields in infinite regions of space. Astrophys. J. 283, 349–362 (1984).
https://doi.org/10.1086/162313
4. T. Amari, J.J. Aly, Magnetic flux ropes: fundamental structures for eruptive phenomena, in Universal Heliophysical Processes, IAU Symposium, vol. 257, ed. by N. Gopalswamy, D.F. Webb (2009), pp. 211–222.
https://doi.org/10.1017/S1743921309029329
5. T. Amari, J.F. Luciani, J.J. Aly, M. Tagger, Plasmoid formation in a single sheared arcade and application to coronal mass ejections. Astron. Astrophys. 306, 913 (1996a)