activity
20112016
most citedThe Influence of the Magnetic Field on Running Penumbral Waves in the Solar Chromosphere

103 citations · 224 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2016★ 100 cited

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.SR2015★ 21 cited

Simulations of Gyrosynchrotron Microwave Emission from an Oscillating 3D Magnetic Loop

Alexey Kuznetsov, Tom Van Doorsselaere, Veronika Reznikova

Radio observations of solar flares often reveal various periodic or quasi-periodic oscillations. Most likely, these oscillations are caused by magnetohydrodynamic (MHD) oscillation…

astro-ph.SR2013★ 103 cited

The Influence of the Magnetic Field on Running Penumbral Waves in the Solar Chromosphere

D. B. Jess, V. E. Reznikova, T. Van Doorsselaere +2

We use images of high spatial and temporal resolution, obtained using both ground- and space-based instrumentation, to investigate the role magnetic field inclination angles play i…

astro-ph.SR2012

Microwave Emission of Supra-arcade Structure associated with M1.6 Limb Flare

Sujin Kim, Hazel Bain, Kiyoto Shibasaki +1

We have investigated a supra-arcade structure, associated with an M1.6 flare, which occurred on the south-east limb on 4th of November 2010. It is observed in microwaves at 17 GHz…

astro-ph.SR2011

The slow magnetoacoustic mode in the flaring loop

Veronika Reznikova, Kiyoto Shibasaki

We studied long duration flare observed with Nobeyama Radioheliograph at frequencies 17 and 34 GHz and with Ramaty High Energy Solar Spectroscopic Imager at 25-50 keV. We found tha…