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Please use this identifier to cite or link to this item: http://hdl.handle.net/10373/1164

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Title: On signatures of twisted magnetic flux tube emergence
Authors: Vargas Domínguez, Santiago
MacTaggart, David
Green, Lucie
van Driel-Gesztelyi, Lidia
Hood, Alan W.
Affiliation: University of Abertay Dundee. School of Computing & Engineering Systems
Keywords: Flux emergence
Photosphere
Issue Date: 2012
Publisher: Springer Verlag
Type: Journal Article
Refereed: peer-reviewed
Rights: Published version (c)Springer Verlag, available from http://dx.doi.org/10.1007/s11207-011-9789-3. The original publication is available at www.springerlink.com
Citation: Vargas Domínguez, S., et al. 2012. On signatures of twisted magnetic flux tube emergence. Solar Physics. 278(1): pp.33-45. Available from http://dx.doi.org/10.1007/s11207-011-9789-3
Abstract: Recent studies of NOAA active region 10953, by Okamoto et al. (Astrophys. J. Lett. 673, 215, 2008; Astrophys. J. 697, 913, 2009), have interpreted photospheric observations of changing widths of the polarities and reversal of the horizontal magnetic field component as signatures of the emergence of a twisted flux tube within the active region and along its internal polarity inversion line (PIL). A filament is observed along the PIL and the active region is assumed to have an arcade structure. To investigate this scenario, Mac- Taggart and Hood (Astrophys. J. Lett. 716, 219, 2010) constructed a dynamic flux emergence model of a twisted cylinder emerging into an overlying arcade. The photospheric signatures observed by Okamoto et al. (2008, 2009) are present in the model although their underlying physical mechanisms differ. The model also produces two additional signatures that can be verified by the observations. The first is an increase in the unsigned magnetic flux in the photosphere at either side of the PIL. The second is the behaviour of characteristic photospheric flow profiles associated with twisted flux tube emergence. We look for these two signatures in AR 10953 and find negative results for the emergence of a twisted flux tube along the PIL. Instead, we interpret the photospheric behaviour along the PIL to be indicative of photospheric magnetic cancellation driven by flows from the dominant sunspot. Although we argue against flux emergence within this particular region, the work demonstrates the important relationship between theory and observations for the successful discovery and interpretation of signatures of flux emergence.
URI: http://hdl.handle.net/10373/1164
ISSN: 0038-0938
Appears in Collections:Computing & Engineering Systems Collection

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