Characteristics of transverse oscillations in a coronal loop arcade

By Erwin Verwichte, Valery M. Nakariakov, L. Ofman, Edward E. DeLuca. 2004

219 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/252f818fbaa322a73d3a5d94652d54ccad3b1ba1

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Citations in the corpus

Coronal Waves and Oscillations (2005, methodology): “The tadpole edges analysed in Verwichte et al. (2005) are marked with letters.”
MHD seismology of coronal loops using the period and damping of quasi-mode kink oscillations (2007, methodology): “More recently, the detection of double mode kink oscillations in several loops in a coronal arcade by Verwichte et al. (2004) has been used by Andries et al. (2005a) to determine the density stratification in those loops.”
Effect of longitudinal magnetic and density inhomogeneity on transversal coronal loop oscillations (2008, background): “These magnetoacoustic oscillations have been observed many times, e.g., Aschwanden et al. (1999a), Aschwanden et al. (2002), Nakariakov et al. (1999) and Verwichte et al. (2004) and have been identified as the standing fast kink mode from MHD wave theory developed by e.g., Edwin & Roberts (1983).”
Decaying and decayless transverse oscillations of a coronal loop (2013, background): “…of transverse oscillations are flare-generated rapidly decaying standing global modes (e.g. Nakariakov et al. 1999) or higher spatial harmonics (Verwichte et al. 2004; De Moortel & Brady 2007; Van Doorsselaere et al. 2007), but they have been observed as propagating waves in quiescent active…”
CORONAL LOOP OSCILLATIONS OBSERVED WITH ATMOSPHERIC IMAGING ASSEMBLY—KINK MODE WITH CROSS-SECTIONAL AND DENSITY OSCILLATIONS (2011, background): “Amazingly, the intensity flux modulation appears to be synchronized with the oscillation amplitude, which is a very interesting property that we have not noticed in previous observations of loop oscillations (e.g., in the 26 cases observed with TRACE; Aschwanden et al. 1999, 2002).”
Detection of Waves in the Solar Corona: Kink or Alfvén? (2008, background): “The typical internal Alfvén speed is about 1000 km s 1 (see, e.g., Verwichte et al. 2004).”
Transverse Oscillations of Coronal Loops (2009, methodology): “They applied their analysis to the two cases of simultaneous observations of the fundamental mode and first overtone reported by Verwichte et al. (2004).”
Coronal loop seismology using multiple transverse loop oscillation harmonics (2007, methodology): “Recently, Verwichte et al. (2004) found two events with signatures of 2 different periodicities in a single loop in an arcade.”
Multiwavelength Studies of MHD Waves in the Solar Chromosphere (2015, background): “…advent of higher sensitivity instrumentation, it has become apparent that not only can eruptive flare events trigger oscillatory phenomena (e.g., Verwichte et al. 2004; Wang and Solanki 2004; De Moortel and Brady 2007; Van Doorsselaere et al. 2007, 2009a; Jess et al. 2008b; Luna et al. 2008;…”
Determination of the Coronal Density Stratification from the Observation of Harmonic Coronal Loop Oscillations (2005, methodology): “Multimode oscillations were detected for the first time by Verwichte et al. (2004).”
Decayless low-amplitude kink oscillations: a common phenomenon in the solar corona? (2015, background): “In some cases, second and third spatial harmonics have been detected (Verwichte et al. 2004; De Moortel & Brady 2007; Van Doorsselaere et al. 2009).”
Hinode observations of transverse waves with flows in coronal loops (2008, background): “…and SOHO data (e.g., Nakariakov et al. 1999; Nakariakov & Ofman 2001; Ofman 2002; De Moortel et al. 2002; Ofman & Wang 2002; Ofman & Thompson 2002; Verwichte et al. 2004; Wang & Solanki 2004; Aschwanden 2005), with recent advances (e.g., Ofman 2007; Wang et al. 2007; Van Doorsselaere et al. 2007;…”
Coronal Seismology by Means of Kink Oscillation Overtones (2009, methodology): “This has first been done by Andries et al. (2005) and Goossens et al. (2006) for the two observations of overtones reported by Verwichte et al. (2004).”
Standing Slow-Mode Waves in Hot Coronal Loops: Observations, Modeling, and Coronal Seismology (2010, methodology): “6 Measured decay time vs. period for the events observed with the BCS reported by Mariska (2006), the SUMER events reported by (Wang et al. 2003b), and the TRACE events reported by Ofman & Aschwanden (2002), Wang & Solanki (2004), and Verwichte et al. (2004).”