arXiv Analytics

Sign in

arXiv:1312.3153 [astro-ph.SR]AbstractReferencesReviewsResources

Observations of a Hybrid Double-Streamer/Pseudostreamer in the Solar Corona

Laurel A. Rachmeler, Sarah J. Platten, Christian Bethge, Daniel B. Seaton, Anthony R. Yeates

Published 2013-12-11, updated 2014-04-03Version 2

We report on the first observation of a single hybrid magnetic structure that contains both a pseudostreamer and a double helmet streamer. This structure was originally observed by the SWAP instrument aboard the PROBA2 satellite between 5 and 10~May~2013. 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 helmet 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 modelling techniques. We describe the topology and dynamic consequences of such a unified structure.

Comments: 19 pages, 4 figures, 2 linked animations, accepted by ApJL
Categories: astro-ph.SR
Related articles: Most relevant | Search more
arXiv:2206.03090 [astro-ph.SR] (Published 2022-06-07)
Observation of Magnetic Switchback in the Solar Corona
arXiv:1204.3787 [astro-ph.SR] (Published 2012-04-17)
Observation and Simulation of Longitudinal Oscillations of an Active Region Prominence
arXiv:1210.6779 [astro-ph.SR] (Published 2012-10-25, updated 2012-10-26)
Observation of an Instability in a 'Quiescent' Prominence