Transverse Oscillations of Coronal Loops

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CORONAL LOOP OSCILLATIONS OBSERVED WITH ATMOSPHERIC IMAGING ASSEMBLY—KINK MODE WITH CROSS-SECTIONAL AND DENSITY OSCILLATIONS (2011, background): “…and observations of coronal seismology can be found in Roberts & Nakariakov (2003), Erdelyi et al. (2003), Roberts (2004), Aschwanden (2004, 2006), Wang (2004), Nakariakov & Verwichte (2005), Banerjee et al. (2007), Andries et al. (2009), Ruderman & Erdelyi (2009), and Taroyan & Erdelyi (2009).”
Multiwavelength Studies of MHD Waves in the Solar Chromosphere (2015, background): “To date, there have been numerous successful applications in the corona (i.e., coronal seismology) with significant focus on fast MHD kink waves (e.g., Nakariakov and Verwichte 2005; Ruderman and Erdélyi 2009; Andries et al. 2009).”
Decayless low-amplitude kink oscillations: a common phenomenon in the solar corona? (2015, background): “In the large-amplitude, rapidly-decaying regime the displacement amplitude reaches several minor radii of the oscillating loop, and the decay time equals two to four periods of the oscillation (see e.g. Ruderman & Erdélyi 2009, for a dedicated review).”