activity
20182022
most citedWhat drives decayless kink oscillations in active region coronal loops on the Sun?

37 citations · 142 across the 7 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2022

A Statistical Comparison of EUV Brightenings Observed by SO/EUI with Simulated Brightenings in Non-potential Simulations

Krzysztof Barczynski, Karen A. Meyer, Louise K. Harra +3

The High Resolution Imager (HRI_EUV) telescope of the Extreme Ultraviolet Imager (EUI) instrument onboard Solar Orbiter has observed EUV brightenings, so-called campfires, as fine-…

astro-ph.SR202214 cited

Plasma composition measurements in an active region from Solar Orbiter/SPICE and Hinode/EIS

David H. Brooks, Miho Janvier, Deborah Baker +28

A key goal of the Solar Orbiter mission is to connect elemental abundance measurements of the solar wind enveloping the spacecraft with EUV spectroscopic observations of their sola…

astro-ph.SR202237 cited

What drives decayless kink oscillations in active region coronal loops on the Sun?

Sudip Mandal, Lakshmi P. Chitta, Patrick Antolin +19

We study here the phenomena of decayless kink oscillations in a system of active region (AR) coronal loops. Using high resolution observations from two different instruments, namel…

astro-ph.SR202122 cited

Solar prominence diagnostics from non-LTE modelling of Mgii h&k line profiles

Aaron W. Peat, Nicolas Labrosse, Brigitte Schmieder +1

Aims: We investigate a new method to for obtaining the plasma parameters of solar prominences observed in the Mgii h&k spectral lines by comparing line profiles from the IRIS satel…

astro-ph.SR202119 cited

Spectro-imagery of an active tornado-like prominence: formation and evolution

Krzysztof Barczynski, Brigitte Schmieder, Aaron W. Peat +3

The nature of flows in tornado-prominences is an open issue. While the AIA imager aboard the Solar Dynamics Observatory (SDO) allowed us to follow the global structure of a tornado…

astro-ph.SR202110 cited

The Formation and Lifetime of Outflows in a Solar Active Region

David H. Brooks, Louise Harra, Stuart D. Bale +4

Active regions are thought to be one contributor to the slow solar wind. Upflows in EUV coronal spectral lines are routinely osberved at their boundaries, and provide the most dire…