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Magnetic topology of active regions and coronal holes: implications for coronal outflows and the solar wind

van Driel-Gesztelyi, L; Culhane, JL; Baker, D; Démoulin, P; Mandrini, CH; DeRosa, ML; Rouillard, AP; ... Vourlidas, A; + view all (2012) Magnetic topology of active regions and coronal holes: implications for coronal outflows and the solar wind. Solar Physics , 281 (1) 237 -262. 10.1007/s11207-012-0076-8. Green open access

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Abstract

During 2-18 January 2008 a pair of low-latitude opposite-polarity coronal holes (CHs) were observed on the Sun with two active regions (ARs) and the heliospheric plasma sheet located between them. We use the Hinode/EUV Imaging Spectrometer (EIS) to locate AR-related outflows and measure their velocities. Solar-Terrestrial Relations Observatory (STEREO) imaging is also employed, as are the Advanced Composition Explorer (ACE) in-situ observations, to assess the resulting impacts on the solar wind (SW) properties. Magnetic-field extrapolations of the two ARs confirm that AR plasma outflows observed with EIS are co-spatial with quasi-separatrix layer locations, including the separatrix of a null point. Global potential-field source-surface modeling indicates that field lines in the vicinity of the null point extend up to the source surface, enabling a part of the EIS plasma upflows access to the SW. We find that similar upflow properties are also observed within closed-field regions that do not reach the source surface. We conclude that some of plasma upflows observed with EIS remain confined along closed coronal loops, but that a fraction of the plasma may be released into the slow SW. This suggests that ARs bordering coronal holes can contribute to the slow SW. Analyzing the in-situ data, we propose that the type of slow SW present depends on whether the AR is fully or partially enclosed by an overlying streamer. © 2012 Springer Science+Business Media B.V.

Type: Article
Title: Magnetic topology of active regions and coronal holes: implications for coronal outflows and the solar wind
Open access status: An open access version is available from UCL Discovery
DOI: 10.1007/s11207-012-0076-8
Publisher version: http://dx.doi.org/10.1007/s11207-012-0076-8
Language: English
Additional information: The final publication is available at link.springer.com
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/1368907
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