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Explaining the Hemispheric Pattern of Filament Chirality.

Authors :
Mackay, Duncan H.
Yeates, Anthony R.
Source :
Proceedings of the International Astronomical Union; Jun2013 Supplement, Vol. 8 Issue S300, p172-175, 4p
Publication Year :
2013

Abstract

Solar filaments are known to exhibit a hemispheric pattern in their chirality, where dextral/sinistral filaments dominate in the northern/southern hemisphere. We show that this pattern may be explained through data driven 3D global magnetic field simulations of the Sun's large-scale magnetic field. Through a detailed comparison with 109 filaments over a 6 month period, the model correctly reproduces the filament chirality and helicity with a 96% agreement. The data driven simulation is extended to run over a full solar cycle, where predictions are made for the spatial and temporal dependence of the hemispheric pattern over the solar cycle. [ABSTRACT FROM PUBLISHER]

Details

Language :
English
ISSN :
17439213
Volume :
8
Issue :
S300
Database :
Complementary Index
Journal :
Proceedings of the International Astronomical Union
Publication Type :
Academic Journal
Accession number :
93466966
Full Text :
https://doi.org/10.1017/S1743921313010934