activity
20182024
most citedObservation of Magnetic Switchback in the Solar Corona

56 citations · 339 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.SR2024★ 6 cited

Kelvin-Helmholtz instability and heating in oscillating loops perturbed by power-law transverse wave drivers

Konstantinos Karampelas, Tom Van Doorsselaere, Mingzhe Guo +2

Instabilities in oscillating loops are believed to be essential for dissipating the wave energy and heating the solar coronal plasma. Our aim is to study the development of the Kel…

astro-ph.SR2023★ 8 cited

Evolution of dynamic fibrils from the cooler chromosphere to the hotter corona

Sudip Mandal, Hardi Peter, Lakshmi Pradeep Chitta +17

Dynamic fibrils (DFs) are commonly observed chromospheric features in solar active regions. Recent observations from the Extreme Ultraviolet Imager (EUI) aboard the Solar Orbiter h…

astro-ph.SR2023★ 17 cited

A multiple spacecraft detection of the 2 April 2022 M-class flare and filament eruption during the first close Solar Orbiter perihelion

M. Janvier, S. Mzerguat, P. R. Young +56

The Solar Orbiter mission completed its first remote-sensing observation windows in the spring of 2022. On 2/4/2022, an M-class flare followed by a filament eruption was seen both…

astro-ph.SR2023★ 14 cited

Influence of the Lower Atmosphere on Wave Heating and Evaporation in Solar Coronal Loops

Mingzhe Guo, Timothy Duckenfield, Tom Van Doorsselaere +3

We model a coronal loop as a three-dimensional magnetic cylinder in a realistic solar atmosphere that extends from the chromosphere to the corona. Kink oscillations, believed ubiqu…

astro-ph.SR2023★ 11 cited

Slow Solar Wind Connection Science during Solar Orbiter's First Close Perihelion Passage

Stephanie L. Yardley, Christopher J. Owen, David M. Long +76

The Slow Solar Wind Connection Solar Orbiter Observing Plan (Slow Wind SOOP) was developed to utilise the extensive suite of remote sensing and in situ instruments on board the ESA…

astro-ph.SR2023★ 25 cited

Temperature of Solar Orbiter/EUI quiet Sun small scale brightenings: evidence for a cooler component

A. Dolliou, S. Parenti, F. Auchère +16

Context: On 2020 May 30, small and short-lived EUV brightenings were observed in the Quiet Sun (QS) during a four minutes sequence by EUI/HRIEUV on board Solar Orbiter. Their physi…

astro-ph.SR2023★ 19 cited

Cut-off of transverse waves through the solar transition region

Gabriel Pelouze, Tom Van Doorsselaere, Konstantinos Karampelas +2

Context. Transverse oscillations are ubiquitously observed in the solar corona, both in coronal loops and open magnetic flux tubes. Numerical simulations suggest that their dissipa…

astro-ph.SR2022★ 16 cited

Signatures of dynamic fibrils at the coronal base: Observations from Solar Orbiter/EUI

Sudip Mandal, Hardi Peter, Lakshmi Pradeep Chitta +20

The solar chromosphere hosts a wide variety of transients, including dynamic fibrils (DFs) that are characterised as elongated, jet-like features seen in active regions, often thro…

astro-ph.SR2022★ 14 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.SR2022★ 37 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.SR2022★ 56 cited

Observation of Magnetic Switchback in the Solar Corona

Daniele Telloni, Gary P. Zank, Marco Stangalini +49

Switchbacks are sudden, large radial deflections of the solar wind magnetic field, widely revealed in interplanetary space by the Parker Solar Probe. The switchbacks' formation mec…

astro-ph.SR2021★ 21 cited

The role of asymmetries in coronal rain formation during thermal non-equilibrium cycles

Gabriel Pelouze, Frédéric Auchère, Karine Bocchialini +4

Context: Thermal non-equilibrium (TNE) produces several observables that can be used to constrain the spatial and temporal distribution of solar coronal heating. Its manifestations…

astro-ph.SR2021★ 24 cited

Linking the Sun to the Heliosphere Using Composition Data and Modelling. A Test Case with a Coronal Jet

Susanna Parenti, Iulia Chifu, Giulio Del Zanna +13

Our understanding of the formation and evolution of the corona and the heliosphere is linked to our capability of properly interpreting the data from remote sensing and in-situ obs…

astro-ph.SR2019★ 12 cited

On the spectroscopic detection of periodic plasma flows in loops undergoing thermal non-equilibrium

Gabriel Pelouze, Frédéric Auchère, Karine Bocchialini +3

Context: Long-period intensity pulsations were recently detected in the EUV emission of coronal loops, and have been attributed to cycles of plasma evaporation and condensation dri…

astro-ph.SR2019★ 5 cited

Comprehensive Determination of the Hinode/EIS Roll Angle

Gabriel Pelouze, Frédéric Auchère, Karine Bocchialini +5

We present a new coalignment method for the EUV Imaging Spectrometer (EIS) on board the Hinode spacecraft. In addition to the pointing offset and spacecraft jitter, this method det…

astro-ph.SR2018★ 54 cited

The Coronal Monsoon: Thermal Nonequilibrium Revealed by Periodic Coronal Rain

F. Auchère, C. froment, E. Soubrié +3

We report on the discovery of periodic coronal rain in an off-limb sequence of {\it Solar Dynamics Observatory}/Atmospheric Imaging Assembly images. The showers are co-spatial and…