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Evolution of the Active Region NOAA 12443 based on magnetic field extrapolations: preliminary results

Published online by Cambridge University Press:  12 September 2017

André Chicrala ,
Renato Sergio Dallaqua ,
Luis Eduardo Antunes Vieira ,
Alisson Dal Lago ,
Jenny Marcela Rodríguez Gómez ,
Judith Palacios ,
Tardelli Ronan Coelho Stekel ,
Joaquim Eduardo Rezende Costa  and
Marlos da Silva Rockenbach
André Chicrala
Affiliation:
National Institute for Space Research, 12227-010, São José dos Campos, Brazil email: andre.chicrala@inpe.br
Renato Sergio Dallaqua
Affiliation:
National Institute for Space Research, 12227-010, São José dos Campos, Brazil email: andre.chicrala@inpe.br
Luis Eduardo Antunes Vieira
Affiliation:
National Institute for Space Research, 12227-010, São José dos Campos, Brazil email: andre.chicrala@inpe.br
Alisson Dal Lago
Affiliation:
National Institute for Space Research, 12227-010, São José dos Campos, Brazil email: andre.chicrala@inpe.br
Jenny Marcela Rodríguez Gómez
Affiliation:
National Institute for Space Research, 12227-010, São José dos Campos, Brazil email: andre.chicrala@inpe.br
Judith Palacios
Affiliation:
Departamento de Física y Matemáticas, Universidad de Alcalá University Campus, Sciences Building, P.O. 28871, Alcalá de Henares, Spain email: judith.palacios@uah.es
Tardelli Ronan Coelho Stekel
Affiliation:
National Institute for Space Research, 12227-010, São José dos Campos, Brazil email: andre.chicrala@inpe.br
Joaquim Eduardo Rezende Costa
Affiliation:
National Institute for Space Research, 12227-010, São José dos Campos, Brazil email: andre.chicrala@inpe.br
Marlos da Silva Rockenbach
Affiliation:
National Institute for Space Research, 12227-010, São José dos Campos, Brazil email: andre.chicrala@inpe.br
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Abstract

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The behavior of Active Regions (ARs) is directly related to the occurrence of some remarkable phenomena in the Sun such as solar flares or coronal mass ejections (CME). In this sense, changes in the magnetic field of the region can be used to uncover other relevant features like the evolution of the ARs magnetic structure and the plasma flow related to it. In this work we describe the evolution of the magnetic structure of the active region AR NOAA12443 observed from 2015/10/30 to 2015/11/10, which may be associated with several X-ray flares of classes C and M. The analysis is based on observations of the solar surface and atmosphere provided by HMI and AIA instruments on board of the SDO spacecraft. In order to investigate the magnetic energy buildup and release of the ARs, we shall employ potential and linear force free extrapolations based on the solar surface magnetic field distribution and the photospheric velocity fields.

Keywords

PhotosphereSunspotsEvolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S328: Living Around Active Stars , October 2016 , pp. 127 - 129
Copyright
Copyright © International Astronomical Union 2017 

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