On signatures of twisted magnetic flux tube emergence

Santiago Vargas Domínguez, David MacTaggart, L. Green, Lidia van Driel-Gesztelyi, Alan W. Hood

Research output: Contribution to journalArticle

  • 10 Citations

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.
Original languageEnglish
Pages (from-to)33–45
Number of pages13
JournalSolar Physics
Volume278
Issue number1
DOIs
StatePublished - 2012

Fingerprint

polarity
signatures
inversions
tubes
magnetic flux
flow characteristics
photosphere
sunspots
cancellation
emerging
filaments
profiles
magnetic fields
sunspot
magnetic field

Cite this

Vargas Domínguez, S., MacTaggart, D., Green, L., van Driel-Gesztelyi, L., & Hood, A. W. (2012). On signatures of twisted magnetic flux tube emergence. Solar Physics, 278(1), 33–45. DOI: 10.1007/s11207-011-9789-3

Vargas Domínguez, Santiago; MacTaggart, David; Green, L.; van Driel-Gesztelyi, Lidia; Hood, Alan W. / On signatures of twisted magnetic flux tube emergence.

In: Solar Physics, Vol. 278, No. 1, 2012, p. 33–45.

Research output: Contribution to journalArticle

@article{753aac77f8a94489a8ce968b09fd474b,
title = "On signatures of twisted magnetic flux tube emergence",
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.",
author = "{Vargas Domínguez}, Santiago and David MacTaggart and L. Green and {van Driel-Gesztelyi}, Lidia and Hood, {Alan W.}",
year = "2012",
doi = "10.1007/s11207-011-9789-3",
volume = "278",
pages = "33–45",
journal = "Solar Physics",
issn = "0038-0938",
publisher = "Springer Netherlands",
number = "1",

}

Vargas Domínguez, S, MacTaggart, D, Green, L, van Driel-Gesztelyi, L & Hood, AW 2012, 'On signatures of twisted magnetic flux tube emergence' Solar Physics, vol 278, no. 1, pp. 33–45. DOI: 10.1007/s11207-011-9789-3

On signatures of twisted magnetic flux tube emergence. / Vargas Domínguez, Santiago; MacTaggart, David; Green, L.; van Driel-Gesztelyi, Lidia; Hood, Alan W.

In: Solar Physics, Vol. 278, No. 1, 2012, p. 33–45.

Research output: Contribution to journalArticle

TY - JOUR

T1 - On signatures of twisted magnetic flux tube emergence

AU - Vargas Domínguez,Santiago

AU - MacTaggart,David

AU - Green,L.

AU - van Driel-Gesztelyi,Lidia

AU - Hood,Alan W.

PY - 2012

Y1 - 2012

N2 - 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.

AB - 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.

U2 - 10.1007/s11207-011-9789-3

DO - 10.1007/s11207-011-9789-3

M3 - Article

VL - 278

SP - 33

EP - 45

JO - Solar Physics

T2 - Solar Physics

JF - Solar Physics

SN - 0038-0938

IS - 1

ER -

Vargas Domínguez S, MacTaggart D, Green L, van Driel-Gesztelyi L, Hood AW. On signatures of twisted magnetic flux tube emergence. Solar Physics. 2012;278(1):33–45. Available from, DOI: 10.1007/s11207-011-9789-3