16 citations · 64 across the 11 of their papers we have counts for
11 papers
Synthetic Fe XIII 1074.7 nm Observations of Torsional Alfvén Waves in Coronal Waveguides
Samuel Skirvin, Richard Morton, Thomas Schad
Torsional Alfvén waves are a promising mechanism for transporting energy through the solar atmosphere, with implications for coronal heating and solar wind acceleration. Recently,…
The Influence of Opacity on Inferred MHD Wave Signatures in the Lower Solar Atmosphere
Samuel J. Skirvin, Samuel D. T. Grant, David B. Jess +8
Magnetohydrodynamic wave activity in small-scale magnetic structures, such as solar pores, provides key insights into energy transport in the lower solar atmosphere. This study pre…
3D MHD wave propagation and energy transport in a simulated solar vortex
Samuel Skirvin, Viktor Fedun, Gary Verth +1
Magnetic flux tubes in the presence of background rotational flows are abundant throughout the solar atmosphere and may act as conduits for MHD waves to transport energy throughout…
Poynting flux of MHD modes in magnetic solar vortex tubes
Samuel Skirvin, Viktor Fedun, Marcel Goossens +2
Magnetic flux tubes in the presence of background rotational flows, known as solar vortex tubes, are abundant throughout the solar atmosphere and may act as conduits for MHD waves…
Modelling the connection between propagating disturbances and solar spicules
Samuel Skirvin, Tanmoy Samanta, Tom Van Doorsselaere
Propagating (intensity) disturbances (PDs) are well reported in observations of coronal loops and polar plumes in addition to recent links with co-temporal spicule activity in the…
Unveiling the True Nature of Plasma Dynamics from the Reference Frame of a Super-penumbral Fibril
W. Bate, D. B. Jess, S. D. T. Grant +11
The magnetic geometry of the solar atmosphere, combined with projection effects, makes it difficult to accurately map the propagation of ubiquitous waves in fibrillar structures. T…
Mode conversion and energy flux absorption in the structured solar atmosphere
Samuel Skirvin, Tom Van Doorsselaere
Context. Structuring in the solar atmosphere, in the form of inhomogeneities transverse to the magnetic field, is believed to play a vital role in wave propagation, conversion, and…
Modelling of transverse oscillations driven by p-modes in short coronal loops
Yuhang Gao, Mingzhe Guo, Tom Van Doorsselaere +2
Recent observations have revealed two types of decayless transverse oscillations in short coronalloops: one with short periods scaling with loop lengths, and the other with longer…
Alfvénic motions arising from asymmetric acoustic wave drivers in solar magnetic structures
Samuel Skirvin, Yuhang Gao, Tom Van Doorsselaere
Alfvénic motions are ubiquitous in the solar atmosphere and their observed properties are closely linked to those of photospheric p-modes. However, it is still unclear how a predom…
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…
II. The effect of axisymmetric and spatially varying equilibria and flow on MHD wave modes: Cylindrical geometry
Samuel Skirvin, Viktor Fedun, Suzana Silva +1
Magnetohydrodynamic (MHD) waves are routinely observed in the solar atmosphere. These waves are important in the context of solar physics as it is widely believed they can contribu…