20 citations · 62 across the 6 of their papers we have counts for
6 papers
The temporal and spatial evolution of MHD wave modes in sunspots
A. B. Albidah, V. Fedun, A. A. Aldhafeeri +8
Through their lifetime sunspots undergo a change in their area and shape and, as they decay, they fragment into smaller structures. Here, for the first time we analyze the spatial…
Ambipolar Diffusion in the Lower Solar Atmosphere: MHD Simulations of a Sunspot
Conor D. MacBride, David B. Jess, Elena Khomenko +1
Magnetohydrodynamic (MHD) simulations of the solar atmosphere are often performed under the assumption that the plasma is fully ionized. However, in the lower solar atmosphere a re…
The Propagation of Coherent Waves Across Multiple Solar Magnetic Pores
S. D. T. Grant, D. B. Jess, M. Stangalini +9
Solar pores are efficient magnetic conduits for propagating magnetohydrodynamic wave energy into the outer regions of the solar atmosphere. Pore observations often contain isolated…
MCALF: Multi-Component Atmospheric Line Fitting
Conor D. MacBride, David B. Jess
Determining accurate velocity measurements from observations of the Sun is of vital importance to solar physicists who are studying the wave dynamics in the solar atmosphere. Weak…
Spectropolarimetric Fluctuations in a Sunspot Chromosphere
M. Stangalini, D. Baker, G. Valori +8
The instrumental advances made in this new era of 4-meter class solar telescopes with unmatched spectropolarimetric accuracy and sensitivity, will enable the study of chromospheric…
Accurately constraining velocity information from spectral imaging observations using machine learning techniques
Conor D. MacBride, David B. Jess, Samuel D. T. Grant +3
Determining accurate plasma Doppler (line-of-sight) velocities from spectroscopic measurements is a challenging endeavour, especially when weak chromospheric absorption lines are o…