activity
20132025
most citedEvidence for the photospheric excitation of incompressible chromospheric waves

108 citations · 431 across the 13 of their papers we have counts for

collaborators

14 papers

math.DS2025

Periodic patterns in simple biological differential delay models

A. Ivanov, S. Shelyag

Periodic patterns in dynamical behaviours of biological models described by simple form differential delay equations are studied. Mathematical models are given by a class of scalar…

astro-ph.SR2024★ 2 cited

Modeling the effects of a lightbridge on oscillations in a solar pore

Luiz A. C. A. Schiavo, Mykola Gordovskyy, Philippa K. Browning +7

Solar pores are ideal magnetic structures for wave propagation and transport of energy radially-outwards across the upper layers of the solar atmosphere. We aim to model the excita…

math.DS2024

Periodic Solutions in a Simple Delay Differential Equation

Anatoli Ivanov, Sergiy Shelyag

Simple form scalar differential equation with delay and nonlinear negative periodic feedback is considered. The existence of several types of slowly oscillating periodic solutions…

astro-ph.SR2022★ 16 cited

Small-scale solar jet formation and their associated waves and instabilities

Samuel Skirvin, Gary Verth, José Juan González-Avilés +7

Studies on small-scale jets' formation, propagation, evolution, and role, such as type I and II spicules, mottles, and fibrils in the lower solar atmosphere's energetic balance, ha…

physics.flu-dyn2022★ 10 cited

New approach for analysing dynamical processes on the surface of photospheric vortex tubes

Yasir Aljohani, Viktor Fedun, Istvan Ballai +3

The majority of studies on multi-scale vortex motions employ a two-dimensional geometry by using a variety of observational and numerical data. This approach limits the understandi…

astro-ph.SR2020★ 30 cited

Solar Vortex Tubes: Vortex Dynamics in the Solar Atmosphere

Suzana S. A. Silva, Viktor Fedun, Gary Verth +2

In this work, a state-of-the-art vortex detection method, Instantaneous Vorticity Deviation, is applied to locate three-dimensional vortex tube boundaries in numerical simulations…

astro-ph.EP2019★ 48 cited

Stellar Surface Magneto-Convection as a Source of Astrophysical Noise III. Sun-as-a-star Simulations and Optimal Noise Diagnostics

H. M. Cegla, C. A. Watson, S. Shelyag +2

Stellar surface magnetoconvection (granulation) creates asymmetries in the observed stellar absorption lines that can subsequently manifest themselves as spurious radial velocities…

astro-ph.SR2018★ 62 cited

Stellar Surface Magneto-Convection as a Source of Astrophysical Noise II. Center-to-Limb Parameterisation of Absorption Line Profiles and Comparison to Observations

H. M. Cegla, C. A. Watson, S. Shelyag +6

Manifestations of stellar activity (such as star-spots, plage/faculae, and convective flows) are well known to induce spectroscopic signals often referred to as astrophysical noise…

astro-ph.SR2018★ 5 cited

Analysis of 3D plasma motions in a chromospheric jet formed due to magnetic reconnection

J. J. González-Avilés, F. S. Guzmán, V. Fedun +4

Within the framework of resistive MHD, implementing the C7 equilibrium atmosphere model and a 3D potential magnetic field realistic configuration, we simulate the formation of a pl…

astro-ph.SR2017★ 24 cited

I. Jet Formation and Evolution due to 3D Magnetic Reconnection

J. J. González-Avilés, F. S. Guzmán, V. Fedun +3

Using simulated data-driven three-dimensional resistive MHD simulations of the solar atmosphere, we show that magnetic reconnection can be responsible of the formation of jets with…

astro-ph.SR2015★ 23 cited

3D simulations of realistic power halos in magneto-hydrostatic sunspot atmospheres: linking theory and observation

Carlos Rijs, S. P. Rajaguru, Damien Przybylski +3

The well-observed acoustic halo is an enhancement in time-averaged Doppler velocity and intensity power with respect to quiet-sun values which is prominent for weak and highly incl…

astro-ph.SR2015★ 32 cited

Ellerman Bombs with Jets: Cause and Effect

A. Reid, M. Mathioudakis, E. Scullion +3

Ellerman Bombs (EBs) are thought to arise as a result of photospheric magnetic reconnection. We use data from the Swedish 1-m Solar Telescope (SST), to study EB events on the solar…

astro-ph.SR2015★ 71 cited

The Dynamics of Rapid Redshifted and Blueshifted Excursions in the Solar Halpha line

D. Kuridze, V. Henriques, M. Mathioudakis +5

We analyse high temporal and spatial resolution time-series of spectral scans of the Halpha line obtained with the CRisp Imaging SpectroPolarimeter (CRISP) instrument mounted on th…

astro-ph.SR2013★ 108 cited

Evidence for the photospheric excitation of incompressible chromospheric waves

R. J. Morton, G. Verth, V. Fedun +2

Observing the excitation mechanisms of incompressible transverse waves is vital for determining how energy propagates through the lower solar atmosphere. We aim to show the connect…