127 citations · 986 across the 31 of their papers we have counts for
31 papers
Decoding the Radial Velocity Signatures of Solar Faculae with 3D MHD Simulations
Florian Kröll, Sowmya Krishnamurthy, Alexander Shapiro +8
We model the solar radial velocity (RV) signal induced by faculae, the dominant contributor to RV variability in Sun-like stars. We use a representative case of a facular patch tra…
Constraining the magnetic vector in the quiet solar photosphere and the impact of instrumental degradation
R. J. Campbell, S. Shelyag, C. Quintero Noda +3
With the advent of next generation high resolution telescopes, our understanding of how the magnetic field is organized in the internetwork (IN) photosphere is likely to advance.We…
Using the Stokes V widths of Fe I lines for diagnostics of the intrinsic solar photospheric magnetic field
M. Gordovskyy, S. Shelyag, P. K. Browning +1
The goal of this study is to explore a novel method for the solar photospheric magnetic field diagnostics using Stokes V widths of different magnetosensitive Fe~I spectral lines. W…
High-resolution spectropolarimetric observations of the temporal evolution of magnetic fields in photospheric bright points
Peter H. Keys, Aaron Reid, Mihalis Mathioudakis +7
Context. Magnetic bright points (MBPs) are dynamic, small-scale magnetic elements often found with field strengths of the order of a kilogauss within intergranular lanes in the pho…
The magnetic properties of photospheric magnetic bright points with high resolution spectropolarimetry
Peter H. Keys, Aaron Reid, Mihalis Mathioudakis +7
Magnetic bright points are small-scale magnetic elements ubiquitous across the solar disk, with the prevailing theory suggesting that they form due to the process of convective col…
Flows and magnetic field structures in reconnection regions of simulations of the solar atmosphere: do flux pile-up models work?
S. Shelyag, Y. E. Litvinenko, V. Fedun +3
We study the process of magnetic field annihilation and reconnection in simulations of magnetised solar photosphere and chromosphere with magnetic fields of opposite polarities and…