Waves in Solar Coronal Loops
Abstract
Recent observations have revealed the ubiquitous presence of magnetohydrodynamic (MHD) waves and oscillations in the solar corona. The aim of this review is to present recent progress in the observational study of four types of wave (or oscillation) phenomena mainly occurring in active region coronal loops, including (i) flare-induced slow mode oscillations, (ii) fast kink mode oscillations, (iii) propagating slow magnetoacoustic waves, and (iv) ubiquitous propagating kink (Alfvenic) waves. This review not only comprehensively outlines various aspects of these waves and coronal seismology, but also highlights the topics that are newly emerging or hotly debated, thus can provide readers a useful guidance on further studies of their interested topics.
Cite
@article{arxiv.1803.11329,
title = {Waves in Solar Coronal Loops},
author = {Tongjiang Wang},
journal= {arXiv preprint arXiv:1803.11329},
year = {2018}
}
Comments
24 pages, 6 figures, published in 2016