443 citations · 3.8k across the 111 of their papers we have counts for
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Unravelling the components of a multi-thermal coronal loop using magnetohydrodynamic seismology
S. Krishna Prasad, D. B. Jess, J. A. Klimchuk +1
Coronal loops, constituting the basic building blocks of the active Sun, serve as primary targets to help understand the mechanisms responsible for maintaining multi-million Kelvin…
Observations and simulations of the Na I D1 line profiles in an M-class solar flare
D. Kuridze, M. Mathioudakis, D. J. Christian +7
We study the temporal evolution of the Na I D1 line profiles in the M3.9 flare SOL2014-06-11T21:03 UT, using high spectral resolution observations obtained with the IBIS instrument…
Departure of high temperature iron lines from the equilibrium state in flaring solar plasmas
Tomoko Kawate, Francis P. Keenan, David B. Jess
The aim of this study is to clarify if the assumption of ionization equilibrium and a Maxwellian electron energy distribution is valid in flaring solar plasmas. We analyze the 2014…
Solar coronal magnetic fields derived using seismology techniques applied to omnipresent sunspot waves
D. B. Jess, V. E. Reznikova, R. S. I. Ryans +9
Sunspots on the surface of the Sun are the observational signatures of intense manifestations of tightly packed magnetic field lines, with near-vertical field strengths exceeding 6…
The effects of transients on photospheric and chromospheric power distributions
T. Samanta, V. M. J. Henriques, D. Banerjee +4
We have observed a quiet Sun region with the Swedish 1-meter Solar Telescope (SST) equipped with CRISP Imaging SpectroPolarimeter. High-resolution, high-cadence, H line scanning…
Time-dependent suppression of oscillatory power in evolving solar magnetic fields
S. Krishna Prasad, D. B. Jess, R. Jain +1
Oscillation amplitudes are generally smaller within magnetically active regions like sunspots and plage, when compared to their surroundings. Such magnetic features, when viewed in…