activity
20112021
most citedCoronal heating by MHD waves

243 citations · 821 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2021★ 24 cited

Novel data analysis techniques in coronal seismology

Sergey A. Anfinogentov, Patrick Antolin, Andrew R. Inglis +7

We review novel data analysis techniques developed or adapted for the field of coronal seismology. We focus on methods from the last ten years that were developed for extreme ultra…

astro-ph.SR2021★ 145 cited

Kink oscillations of coronal loops

V. M. Nakariakov, S. A. Anfinogentov, P. Antolin +13

Kink oscillations of coronal loops, i.e., standing kink waves, is one of the most studied dynamic phenomena in the solar corona. The oscillations are excited by impulsive energy re…

astro-ph.SR2020★ 243 cited

Coronal heating by MHD waves

Tom Van Doorsselaere, Abhishek K. Srivastava, Patrick Antolin +9

The heating of the solar chromosphere and corona to the observed high temperatures, imply the presence of ongoing heating that balances the strong radiative and thermal conduction…

astro-ph.SR2020★ 76 cited

Magnetohydrodynamic Fast Sausage Waves in the Solar Corona

B. Li, P. Antolin, M. -Z. Guo +4

Characterized by cyclic axisymmetric perturbations to both the magnetic and fluid parameters, magnetohydrodynamic fast sausage modes (FSMs) have proven useful for solar coronal sei…

astro-ph.SR2020★ 44 cited

Solar Bayesian Analysis Toolkit -- a new Markov chain Monte Carlo IDL code for Bayesian parameter inference

Sergey A. Anfinogentov, Valery M. Nakariakov, David J. Pascoe +1

We present the Solar Bayesian Analysis Toolkit (SoBAT) which is a new easy to use tool for Bayesian analysis of observational data, including parameter inference and model comparis…

astro-ph.SR2020★ 11 cited

Coronal Density and Temperature Profiles Calculated by Forward Modeling EUV Emission Observed by SDO/AIA

D. J. Pascoe, A. Smyrli, T. Van Doorsselaere

We present a model for the intensity of optically thin EUV emission for a plasma atmosphere. We apply our model to the solar corona as observed using the six optically thin EUV cha…