92 citations · 847 across the 31 of their papers we have counts for
29 papers
Formation Dynamics of a Rotating Solar Spicule-like Event and Associated Energy-Mass Transport
Liufan Gong, Lei Ni, Guanchong Cheng +3
We performed three-dimensional radiative magnetohydrodynamic(3D RMHD) simulations in an upward-directed (positive-polarity) open magnetic field with an initial background strength…
Energy and mass transport associated with impulsive spicular flows in solar coronal holes
Lei Ni, Jun Lin, Tanmoy Samanta +3
How the solar atmosphere is heated from a temperature of about \,K in the lower atmosphere to about \,MK in the corona has challenged the astrophysical community…
Solar Flare Prediction Using Magnetic Field Diagnostics Above the Photosphere
M. B. Korsos, M. K. Georgoulis, N. Gyenge +7
In this article, we present the application of the weighted horizontal gradient of magnetic field (WGM) flare prediction method to 3-dimensional (3D) extrapolated magnetic configur…
Science Requirement Document (SRD) for the European Solar Telescope (EST) (3rd Edition, December 2025)
Rolf Schlichenmaier, Luis R. Bellot Rubio, Manuel Collados Vera +31
The European Strategy Forum on Research Infrastructures (ESFRI) included the European Solar Telescope (EST) as an ESFRI Project in its 2016 Roadmap and confirmed this status in 202…
Magnetic Rayleigh-Taylor Instability at a Contact Discontinuity With Oblique Magnetic Field
E. Vickers, I. Ballai, R. Erdélyi
Aims: In the present work we investigate the nature of the magnetic Rayleigh-Taylor instability at a density interface permeated by an oblique, homogeneous magnetic field in an inc…
Varying Driver Velocity Fields in Photospheric MHD Wave Simulations
A. J. Leonard, S. J. Mumford, V. Fedun +1
Torsional motions are ubiquitous in the solar atmosphere. In this work, we perform 3D numerical simulations which mimic a vortex-type photospheric driver with a Gaussian spatial pr…
Magnetic shocks and substructures excited by torsional Alfvén wave interactions in merging expanding flux tubes
B. Snow, V. Fedun, F. A. Gent +2
Vortex motions are frequently observed on the solar photosphere. These motions may play a key role in the transport of energy and momentum from the lower atmosphere into the upper…
On the evolution of pre-flare patterns of a 3-dimensional model of AR 11429
M. B. Korsos, S. Poedts, N. Gyenge +6
We apply a novel pre-flare tracking of sunspot groups towards improving the estimation of flare onset time by focusing on the evolution of the 3D magnetic field construction of AR…
An application of the weighted horizontal magnetic gradient to solar compact and eruptive events
M. B. Korsos, Michael S. Ruderman, R. Erdelyi
We propose to apply the weighted horizontal magnetic gradient (), introduced in Korsos et al (2015), for analysing the pre-flare and pre-CME behaviour and evolution of Acti…
Dissipative instabilities in a partially ionised prominence plasma slab: II. The effect of compressibility
J. F. Mather, I. Ballai, R. Erdelyi
This present study deals with the dissipative instability that appears in a compressible partially ionised plasma slab embedded in a uniform magnetic field, modelling the state of…
IRIS Burst Spectra Co-Spatial To A Quiet-Sun Ellerman-Like Brightening
C. J. Nelson, N. Freij, A. Reid +3
Ellerman bombs (EBs) have been widely studied over the past two decades; however, only recently have counterparts of these events been observed in the quiet-Sun. The aim of this ar…
An Inside Look at Sunspot Oscillations with Higher Azimuthal Wavenumbers
David B. Jess, Tom Van Doorsselaere, Gary Verth +7
Solar chromospheric observations of sunspot umbrae offer an exceptional view of magneto-hydrodynamic wave phenomena. In recent years, a wealth of wave signatures related to propaga…
On The Relationship Between Magnetic Cancellation and UV Burst Formation
C. J. Nelson, J. G. Doyle, R. Erdelyi
Burst-like events with signatures in the UV are often observed co-spatial to strong line-of-sight photospheric magnetic fields. Several authors, for example, have noted the spatial…
Wave Damping Observed in Upwardly Propagating Sausage-mode Oscillations contained within a Magnetic Pore
S. D. T. Grant, D. B. Jess, M. G. Moreels +8
We present observational evidence of compressible magnetohydrodynamic wave modes propagating from the solar photosphere through to the base of the transition region in a solar magn…
On flare predictability based on sunspot group evolution
Marianna Korsos, Andras Ludmany, Robert Erdelyi +1
The forecast method introduced by Korsós et al.(2014) is generalised from the horizontal magnetic gradient (GM), defined between two opposite polarity spots, to all spots within an…
Small-Scale Structuring Of Ellerman Bombs at Solar Limb
C. J. Nelson, E. M. Scullion, J. G. Doyle +2
Ellerman bombs (EBs) have been widely studied in recent years due to their dynamic, explosive nature and apparent links to the underlying photospheric magnetic field implying that…
A statistical study of transverse oscillations in a quiescent prominence
A. Hillier, R. J. Morton, R. Erdélyi
The launch of the Hinode satellite has allowed for seeing-free observations at high-resolution and high-cadence making it well suited to study the dynamics of quiescent prominences…
Characteristics of transverse waves in chromospheric mottles
D. Kuridze, G. Verth, M. Mathioudakis +5
Using data obtained by the high temporal and spatial resolution Rapid Oscillations in the Solar Atmosphere (ROSA) instrument on the Dunn Solar Telescope, we investigate at an unpre…
Magnetohydrostatic equilibrium. I: Three-dimensional open magnetic flux tube in the stratified solar atmosphere
Frederick Armstrong Gent, Viktor Fedun, Stuart John Mumford +1
A single open magnetic flux tube spanning the solar photosphere (solar radius R) and the lower corona (R + 10 Mm) is modelled in magnetohydrostatic equilibrium within a realistic s…
Observational Evidence of Sausage-Pinch Instability in Solar Corona by SDO/AIA
A. K. Srivastava, R. Erdélyi, Durgesh Tripathi +3
We present the first observational evidence of the evolution of sausage-pinch instability in Active Region 11295 during a prominence eruption using data recorded on 12 September 20…
On standing sausage waves in photospheric magnetic waveguides
I. Dorotovic, R. Erdelyi, N. Freij +2
By focusing on the oscillations of the cross-sectional area and the intensity of magnetic waveguides located in the lower solar atmosphere, we aim to detect and identify magnetohyd…
Magneto-seismology of solar atmospheric loops by means of longitudinal oscillations
M. Luna-Cardozo, G. Verth, R. Erdélyi
There is increasingly strong observational evidence that slow magnetoacoustic modes arise in the solar atmosphere. Solar magneto-seismology is a novel tool to derive otherwise dire…
Vortices in the solar photosphere
S. Shelyag, V. Fedun, R. Erdélyi +2
Using numerical simulations of the magnetised solar photosphere and radiative diagnostics of the simulated photospheric models, we further analyse the physical nature of magnetic p…
Determination of sub-resolution structure of jet by solar magnetoseismology
R. J. Morton, G. Verth, J. A. McLaughlin +1
A thin dark thread is observed in a UV/EUV solar jet in the 171A, 193A and 211A and partially in 304A. The dark thread appears to originate in the chromosphere but its temperature…