Filament Connectivity and “Reconnection”
2013 ◽
Vol 8
(S300)
◽
pp. 412-413
Keyword(s):
AbstractStable long lived solar filaments during their lives can approach each other, merge, and form circular structures. Since filaments follow large scale polarity inversion lines of the photospheric magnetic field, their evolution reflects changes of the photospheric field distribution. On the other hand, filament interaction depends on their internal magnetic structure reviled in particular by filament chirality. Possibility of magnetic field line reconnection of neighbor filaments is discussed. Many examples of connectivity changes in a course of photospheric field evolution were found in our analysis of daily Hα filtergrams for the period of maximum activity of the solar cycle 23.
2014 ◽
Vol 54
(7)
◽
pp. 953-958
◽
Keyword(s):
2013 ◽
Vol 8
(S300)
◽
pp. 172-175
2006 ◽
Vol 46
(6)
◽
pp. 701-707
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Keyword(s):
Keyword(s):
1998 ◽
Vol 167
◽
pp. 493-496
2016 ◽
Vol 12
(S328)
◽
pp. 93-100
◽
Keyword(s):
Keyword(s):
1975 ◽
Vol 68
◽
pp. 19-21
Keyword(s):
2012 ◽
Vol 758
(1)
◽
pp. 61
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