Simulation of sigmoid structure and filament eruption of AR11283 using a three-dimensional data-driven magnetohydrodynamic model. Issue Volume 8:Issue S300(2013) (6th January 2014)

Record Type:: Journal Article
Title:: Simulation of sigmoid structure and filament eruption of AR11283 using a three-dimensional data-driven magnetohydrodynamic model. Issue Volume 8:Issue S300(2013) (6th January 2014)
Main Title:: Simulation of sigmoid structure and filament eruption of AR11283 using a three-dimensional data-driven magnetohydrodynamic model
Authors:: Wu, S. T.
Jiang, Chaowei
Feng, Xueshang
Hu, Qiang
Liu, Yang
Abstract:: Abstract: This paper describes an MHD simulation of an observed Sigmoid in AR 11283 from its formation to eruption. The Non-linear Force Free MHD model (Jiang and Feng, 2012) and the data-driven active region evolution model (Wu et al ., 2006; Jiang et al . 2013) together with the SDO/HMI magnetograms are used. We show the successful simulation results of the eruption of a flux-rope structure.
Is Part Of:: Proceedings of the International Astronomical Union. Volume 8:Issue S300(2013)
Journal:: Proceedings of the International Astronomical Union
Issue:: Volume 8:Issue S300(2013)
Issue Display:: Volume 8, Issue 300 (2013)
Year:: 2013
Volume:: 8
Issue:: 300
Issue Sort Value:: 2013-0008-0300-0000
Page Start:: 466
Page End:: 467
Publication Date:: 2014-01-06
Subjects:: Sigmoid, -- MHD Simulation, -- Active Region, -- Magnetogram
Astronomy -- Congresses
Astronomy -- Periodicals
520
Journal URLs:: http://journals.cambridge.org/action/displayJournal?jid=IAU ↗
DOI:: 10.1017/S1743921313011587 ↗
Languages:: English
ISSNs:: 1743-9213
Deposit Type:: Legaldeposit
View Content:: Available online (eLD content is only available in our Reading Rooms) ↗
Physical Locations:: British Library HMNTS - ELD Digital store
Ingest File:: 4723.xml