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Observation of small scale reconnection role in undulated flux tube emergence

  • E. Pariat
  • , G. Aulanier
  • , B. Schmieder
  • , M. K. Georgoulis
  • , D. M. Rust
  • , P. N. Bernasconi
  • LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique
  • Johns Hopkins University Applied Physics Laboratory

Research output: Contribution to journalConference articlepeer-review

Abstract

With Flare Genesis Experiment (FGE), a balloon borne observatory launched in Antarctica on January 2000, series of high spatial resolution vector magnetograms, Dopplergrams, and Hα filtergrams have been obtained in an emerging active region (AR 8844). We performed a linear force-free field extrapolation of the field above the photosphere. The analysis of the chromospheric magnetic topology reveals the existence of undulated low-lying field lines, presenting a 'sea-serpent' shape. These field lines are passing through several "Bald Patches" regions (BPs are regions where the vector magnetic field is tangential to the photosphere). These separatrice field lines are thus connected to the photosphere. The undulation spectrum leads us to suppose that the undulations are due to the Parker instability. In addition, these undulated field lines are highly associated with many shortlived and small-scale Hα brightenings called 'Ellerman bombs', which are likely to be due to magnetic reconnections along the BP separatrices. This observation permits us to conjecture that reconnection plays a key role in the flux tube emergence process. Arch filament systems and active region coronal loops do not result from the smooth emergence of large scale Ω loops, but rather from the rise of flat undulated flux tubes which get released from their photospheric anchorage by reconnection at BPs.

Original languageEnglish
Pages (from-to)429-432
Number of pages4
JournalEuropean Space Agency, (Special Publication) ESA SP
Issue number596
Publication statusPublished - 1 Dec 2005
Externally publishedYes
EventInternational Scientific Conference on Chromospheric and Coronal Magnetic Fields - Katlenburg - Lindau, Germany
Duration: 30 Aug 20052 Sept 2005

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