Observations of a hybrid double-streamer/pseudostreamer in the solar corona.

We report on the first observation of a single hybrid magnetic structure that contains both a pseudostreamer and a double streamer. This structure was originally observed by the SWAP instrument on board the PROBA2 satellite between 2013 May 5 and 10. It consists of a pair of filament channels near t...

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Bibliographic Details
Published in:The Astrophysical Journal
Main Authors: Rachmeler, L. A., Platten, S. J., Bethge, C., Seaton, D. B., Yeates, A. R.
Format: Article in Journal/Newspaper
Language:unknown
Published: IOP Publishing 2014
Subjects:
Online Access:http://dro.dur.ac.uk/13218/
http://dro.dur.ac.uk/13218/1/13218.pdf
https://doi.org/10.1088/2041-8205/787/1/L3
Description
Summary:We report on the first observation of a single hybrid magnetic structure that contains both a pseudostreamer and a double streamer. This structure was originally observed by the SWAP instrument on board the PROBA2 satellite between 2013 May 5 and 10. It consists of a pair of filament channels near the south pole of the Sun. On the western edge of the structure, the magnetic morphology above the filaments is that of a side-by-side double streamer, with open field between the two channels. On the eastern edge, the magnetic morphology is that of a coronal pseudostreamer without the central open field. We investigated this structure with multiple observations and modeling techniques. We describe the topology and dynamic consequences of such a unified structure.