Slow-mode standing waves observed by SUMER in hot coronal loops

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Standing Slow-Mode Waves in Hot Coronal Loops: Observations, Modeling, and Coronal Seismology (2010, methodology): “Instead, Wang et al. (2003b) proposed a scenario to explain the origin of this phase propagation by excitation of standing slow waves in coronal loops with the (multithreaded) fine structure.”
Vertical oscillations of a coronal loop observed by TRACE (2004, methodology): “Later, hot loop oscillations in Doppler shifts with periods on the order of 20 min were detected by the SUMER spectrometer onboard SOHO, and interpreted in terms of the standing slow mode (e.g. Wang et al. 2002, 2003; Ofman & Wang 2002).”
Hot coronal loop oscillations observed with SUMER: Examples and statistics (2003, methodology): “Various lines of evidence indicating that they are compressive slow magnetoacoustic standing waves are presented, thus supporting the conclusions reached by Wang et al. (2003).”
The EUV Imaging Spectrometer for Hinode (2007, background): “Spectroscopic observations of oscillations in coronal loops have been made in flaring and post flare conditions (Wang et al., 2002, 2003), while on a larger scale spectroscopic observations of EIT waves in the corona have been pioneered by Harra and Sterling (2003).”
Coronal Waves and Oscillations (2005, background): “Recently, Doppler shift and intensity oscillations were discovered in coronal loops observed in the far UV Fexix and Fexxi emission lines with SOHO/SUMER (Wang et al. 2002, 2003).”