Study of magnetic flux emergence and related activity in active region NOAA 10314
We study the extremely complex active region (AR) NOAA 10314, that was observed from March 13-19, 2003. This AR was the source of several energetic events, among them two major (X class) flares, along a few days. We follow the evolution of this AR since the very first stages of its emergence. From t...
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| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_02731177_v51_n10_p1834_Poisson |
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todo:paper_02731177_v51_n10_p1834_Poisson2023-10-03T15:15:43Z Study of magnetic flux emergence and related activity in active region NOAA 10314 Poisson, M. López Fuentes, M. Mandrini, C.H. Démoulin, P. Pariat, E. Magnetic flux emergence Magnetic helicity injection Solar active regions Active regions Computation techniques Flux emergence Flux tubes Local correlation tracking Magnetic flux tube Magnetic helicity Solar active regions Solar energy Tubes (components) Magnetic flux We study the extremely complex active region (AR) NOAA 10314, that was observed from March 13-19, 2003. This AR was the source of several energetic events, among them two major (X class) flares, along a few days. We follow the evolution of this AR since the very first stages of its emergence. From the photospheric evolution of the magnetic polarities observed with SOHO/MDI we infer the morphology of the flux tube that originates the AR. Using a computation technique that combines Local Correlation Tracking with magnetic induction constrains, we compute the rate of magnetic helicity injection at the photosphere during the observed evolution. From our results we conclude that the AR originated by the emergence of a severely deformed magnetic flux tube having a dominantly positive magnetic helicity.© 2012 COSPAR. Published by Elsevier Ltd. All rights reserved. Fil:Poisson, M. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:López Fuentes, M. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Mandrini, C.H. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_02731177_v51_n10_p1834_Poisson |
| institution |
Universidad de Buenos Aires |
| institution_str |
I-28 |
| repository_str |
R-134 |
| collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
| topic |
Magnetic flux emergence Magnetic helicity injection Solar active regions Active regions Computation techniques Flux emergence Flux tubes Local correlation tracking Magnetic flux tube Magnetic helicity Solar active regions Solar energy Tubes (components) Magnetic flux |
| spellingShingle |
Magnetic flux emergence Magnetic helicity injection Solar active regions Active regions Computation techniques Flux emergence Flux tubes Local correlation tracking Magnetic flux tube Magnetic helicity Solar active regions Solar energy Tubes (components) Magnetic flux Poisson, M. López Fuentes, M. Mandrini, C.H. Démoulin, P. Pariat, E. Study of magnetic flux emergence and related activity in active region NOAA 10314 |
| topic_facet |
Magnetic flux emergence Magnetic helicity injection Solar active regions Active regions Computation techniques Flux emergence Flux tubes Local correlation tracking Magnetic flux tube Magnetic helicity Solar active regions Solar energy Tubes (components) Magnetic flux |
| description |
We study the extremely complex active region (AR) NOAA 10314, that was observed from March 13-19, 2003. This AR was the source of several energetic events, among them two major (X class) flares, along a few days. We follow the evolution of this AR since the very first stages of its emergence. From the photospheric evolution of the magnetic polarities observed with SOHO/MDI we infer the morphology of the flux tube that originates the AR. Using a computation technique that combines Local Correlation Tracking with magnetic induction constrains, we compute the rate of magnetic helicity injection at the photosphere during the observed evolution. From our results we conclude that the AR originated by the emergence of a severely deformed magnetic flux tube having a dominantly positive magnetic helicity.© 2012 COSPAR. Published by Elsevier Ltd. All rights reserved. |
| format |
JOUR |
| author |
Poisson, M. López Fuentes, M. Mandrini, C.H. Démoulin, P. Pariat, E. |
| author_facet |
Poisson, M. López Fuentes, M. Mandrini, C.H. Démoulin, P. Pariat, E. |
| author_sort |
Poisson, M. |
| title |
Study of magnetic flux emergence and related activity in active region NOAA 10314 |
| title_short |
Study of magnetic flux emergence and related activity in active region NOAA 10314 |
| title_full |
Study of magnetic flux emergence and related activity in active region NOAA 10314 |
| title_fullStr |
Study of magnetic flux emergence and related activity in active region NOAA 10314 |
| title_full_unstemmed |
Study of magnetic flux emergence and related activity in active region NOAA 10314 |
| title_sort |
study of magnetic flux emergence and related activity in active region noaa 10314 |
| url |
http://hdl.handle.net/20.500.12110/paper_02731177_v51_n10_p1834_Poisson |
| work_keys_str_mv |
AT poissonm studyofmagneticfluxemergenceandrelatedactivityinactiveregionnoaa10314 AT lopezfuentesm studyofmagneticfluxemergenceandrelatedactivityinactiveregionnoaa10314 AT mandrinich studyofmagneticfluxemergenceandrelatedactivityinactiveregionnoaa10314 AT demoulinp studyofmagneticfluxemergenceandrelatedactivityinactiveregionnoaa10314 AT pariate studyofmagneticfluxemergenceandrelatedactivityinactiveregionnoaa10314 |
| _version_ |
1807314597276811264 |