IAFE   05512
INSTITUTO DE ASTRONOMIA Y FISICA DEL ESPACIO
Unidad Ejecutora - UE
artículos
Título:
Correcting the effect of magnetic tongues on the tilt angle of bipolar active regions
Autor/es:
POISSON, M.; DÉMOULIN, P.; LÓPEZ FUENTES, M. C.; MACCORMACK, C.; LÓPEZ FUENTES, M. C.; MACCORMACK, C.; MANDRINI, C. H.; MANDRINI, C. H.; POISSON, M.; DÉMOULIN, P.
Revista:
ASTRONOMY AND ASTROPHYSICS
Editorial:
EDP SCIENCES S A
Referencias:
Lugar: Paris; Año: 2020 vol. 633
ISSN:
0004-6361
Resumen:
Context. The magnetic polarities of bipolar active regions (ARs) exhibit elongations in line-of-sight magnetograms during theiremergence. These elongations are referred to as magnetic tongues and attributed to the presence of twist in the emerging magneticflux-ropes (FRs) that form ARs.Aims. The presence of magnetic tongues affects the measurement of any AR characteristic that depends on its magnetic flux distribution.The AR tilt-angle is one of them. We aim to develop a method to isolate and remove the flux associated with the tongues todetermine the AR tilt-angle with as much precision as possible.Methods. As a first approach, we used a simple emergence model of a FR. This allowed us to develop and test our aim based on amethod to remove the effects of magnetic tongues. Then, using the experience gained from the analysis of the model, we applied ourmethod to photospheric observations of bipolar ARs that show clear magnetic tongues.Results. Using the developed procedure on the FR model, we can reduce the deviation in the tilt estimation by more than 60%. Nextwe illustrate the performance of the method with four examples of bipolar ARs selected for their large magnetic tongues. The newmethod efficiently removes the spurious rotation of the bipole. This correction is mostly independent of the method input parametersand significant since it is larger than all the estimated tilt errors.Conclusions. We have developed a method to isolate the magnetic flux associated with the FR core during the emergence of bipolarARs. This allows us to compute the AR tilt-angle and its evolution as precisely as possible. We suggest that the high dispersionobserved in the determination of AR tilt-angles in studies that massively compute them from line-of sight magnetograms can bepartly due to the existence of magnetic tongues whose presence is not sufficiently acknowledged.