activity
20222026
most citedObservation of Magnetic Switchback in the Solar Corona

56 citations · 101 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2026

Polarization of decayless kink oscillations in a 3D MHD coronal loop model

Sudip Mandal, Cosima Breu, Hardi Peter

Decayless kink oscillations are frequently observed in solar coronal loops and are considered potential contributors to coronal heating. Despite the ubiquity of this wave phenomeno…

astro-ph.SR2025

A self-consistent 3D MHD model producing a solar blowout jet

Yajie Chen, Hardi Peter, Damien Przybylski +2

Context. Solar blowout jets are a distinct subclass of ubiquitous extreme-ultraviolet (EUV) and X-ray coronal jets. Aims. Most existing models of blowout jets prescribe an initial…

astro-ph.SR2025★ 2 cited

Anomalous cross-field motions of solar coronal loops

Sudip Mandal, Hardi Peter, James A. Klimchuk +1

Here, we present several examples of unusual evolutionary patterns in solar coronal loops that resemble cross-field drift motions. These loops were simultaneously observed from two…

astro-ph.SR2024

Bidirectional propagating brightenings in arch filament systems observed by Solar Orbiter/EUI

Yajie Chen, Sudip Mandal, Hardi Peter +1

Arch filament systems (AFSs) are chromospheric and coronal manifestations of emerging magnetic flux. Using high spatial resolution observations taken at a high cadence by the Extre…

astro-ph.SR2024

Investigating coronal loop morphology and dynamics from two vantage points

Sudip Mandal, Hardi Peter, James A. Klimchuk +9

Coronal loops serve as the fundamental building blocks of the solar corona. Therefore, comprehending their properties is essential in unraveling the dynamics of the Sun's upper atm…

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★ 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★ 7 cited

Slow solar wind sources. High-resolution observations with a quadrature view

Krzysztof Barczynski, Louise Harra, Conrad Schwanitz +16

The origin of the slow solar wind is still an open issue. One possibility that has been suggested is that upflows at the edge of an active region can contribute to the slow solar w…

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★ 1 cited

SPICE PSF Correction: General Framework and Capability Demonstration

Joseph E. Plowman, Frédéric Auchère, Regina Aznar Cuadrado +5

We present a new method of removing PSF artifacts and improving the resolution of multidimensional data sources including imagers and spectrographs. Rather than deconvolution, whic…

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…