activity
20092023
most citedMagnetic Reconnection along Quasi-Separatrix Layers as a Driver of Ubiquitous Active Region Outflows

126 citations · 1.2k across the 37 of their papers we have counts for

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Showing 2021Show all

7 papers · 1 filter

astro-ph.SR2021★ 21 cited

Extending the FIP bias sample to magnetically active stars. Challenging the FIP bias paradigm?

B. Seli, K. Oláh, L. Kriskovics +6

The different elemental abundances of the photosphere and the corona are striking features of not only the Sun, but other stars as well. This phenomenon is known as the FIP effect…

astro-ph.SR2021★ 12 cited

Evolution of Plasma Composition in an Eruptive Flux Rope

Deborah Baker, Lucie M. Green, David H. Brooks +8

Magnetic flux ropes are bundles of twisted magnetic field enveloping a central axis. They harbor free magnetic energy and can be progenitors of coronal mass ejections (CMEs), but i…

astro-ph.SR2021★ 14 cited

On the Origin of Magnetic Pertubations associated with the FIP effect

M. Murabito, M. Stangalini, D. Baker +9

In \citet{Stangalini20} and \citet{Deb20}, magnetic oscillations were detected in the chromosphere of a large sunspot and found to be linked to the coronal locations where a First…

astro-ph.SR2021★ 7 cited

Plasma Upflows Induced by Magnetic Reconnection Above an Eruptive Flux Rope

Deborah Baker, Teodora Mihailescu, Pascal Demoulin +6

One of the major discoveries of Hinode's Extreme-ultraviolet Imaging Spectrometer (EIS) is the presence of upflows at the edges of active regions. As active regions are magneticall…

astro-ph.SR2021★ 9 cited

Widespread Occurrence of High-Velocity Upflows in Solar Active Regions

S. L. Yardley, D. H. Brooks, D. Baker

We performed a systematic study of 12 active regions (ARs) with a broad range of areas, magnetic flux and associated solar activity in order to determine whether there are upflows…

astro-ph.SR2021★ 28 cited

The Evolution of Plasma Composition During a Solar Flare

Andy S. H. To, David M. Long, Deborah Baker +4

We analyse the coronal elemental abundances during a small flare using Hinode/EIS observations. Compared to the pre-flare elemental abundances, we observed a strong increase in cor…