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Physical Processes Involved in the EUV “Surge” Event of 9 May 2012

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Abstract

We study an extreme ultraviolet (EUV) confined ejection observed on 9 May 2012 in Active Region (AR) NOAA 11476. For the analysis we use observations in multiple wavelengths (EUV, X-rays, H\(\upalpha\), and magnetograms) from a variety of ground- and space-based instruments. The magnetic configuration showed two rotating bipoles within the following polarity of the AR. This evolution was present some tens of hours before the studied event and continued thereafter. During this period, the magnetic flux of both bipoles continuously decreased. A mini-filament with a length of \({\approx}\,30''\) lay along the photospheric inversion line of the largest bipole. The mini-filament was observed to erupt, accompanied by an M4.7 flare (SOL20120509T12:23:00). This injected dense material as well as twist along closed loops in the form of a very broad ejection whose morphology resembled that of typical H\(\upalpha\) surges. We conclude that the flare and eruption can be explained as due to two reconnection processes, one occurring below the erupting mini-filament, and another above it. This second process injects the mini-filament plasma within the reconnected closed loops linking the main AR polarities. By analyzing the magnetic topology using a force-free model of the coronal field, we identify the location of quasi-separatix layers, where reconnection is prone to occur, and present a detailed interpretation of the chromospheric and coronal eruption observations. In particular, this event, in contrast to what has been proposed in several models explaining surges and/or jets, is not produced by magnetic flux emergence, but by magnetic flux cancellation accompanied by the rotation of the bipoles. In fact, the conjunction of these two processes, flux cancellation and bipole rotations, is at the origin of a series of events, homologous to the event we analyze in this article, which occurred in AR 11476 from 8 to 10 May 2012.

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Acknowledgements

The authors are grateful for the insightful referee, who stimulated us to improve several parts of the manuscript. The authors would like to thank Carlos Francile from the Astronomical Observatory Felix Aguilar, University of San Juan, for his invaluable help in the processing of HASTA data. MLF, CHM and GC are members of the Carrera del Investigador Científico of the Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) of Argentina. MP and FL are CONICET Fellows. MP, MLF, GC and CHM acknowledge financial support from the Argentinean grants PICT 2012-0973 (ANPCyT), UBACyT 20020130100321 and PIP 2012-01-403 (CONICET).

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Authors and Affiliations

  1. Instituto de Astronomía y Física del Espacio (IAFE), CONICET-UBA, Buenos Aires, Argentina

    Marcelo López Fuentes, Cristina H. Mandrini, Mariano Poisson, Germán Cristiani & Maria Luisa Luoni

  2. Facultad de Ciencias Exactas y Naturales (FCEN), UBA, Buenos Aires, Argentina

    Cristina H. Mandrini & Germán Cristiani

  3. LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Univ. Paris Diderot, Sorbonne Paris Cité, 5 place Jules Janssen, Meudon, 92195, Paris, France

    Pascal Démoulin

  4. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio (ICATE), CONICET, San Juan, Argentina

    Fernando M. López

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  1. Marcelo López Fuentes
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  3. Mariano Poisson
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Correspondence to Marcelo López Fuentes.

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López Fuentes, M., Mandrini, C.H., Poisson, M. et al. Physical Processes Involved in the EUV “Surge” Event of 9 May 2012. Sol Phys 293, 166 (2018). https://doi.org/10.1007/s11207-018-1384-4

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