3 papers
astro-ph.SR2016
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…
astro-ph.SR2016
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…
astro-ph.SR2015
Wave Damping Observed in Upwardly Propagating Sausage-mode Oscillations contained within a Magnetic Pore
S. D. T. Grant, D. B. Jess, M. G. Moreels +8
We present observational evidence of compressible magnetohydrodynamic wave modes propagating from the solar photosphere through to the base of the transition region in a solar magn…