Transverse oscillations in coronal loops observed with TRACE – I. An Overview of Events, Movies, and a Discussion of Common Properties and Required Conditions

By C. Schrijver, Markus J. Aschwanden, A. Title. 2001

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In Astronomy and Astrophysics

Citations in the corpus

Coronal Waves and Oscillations (2005, background): “However, there can be higher spatial harmonics observed (Schrijver et al. 2002).”
The solar magnetic field (2006, background): “[573, 574]) and slow mode type compressional oscillations at even longer frequencies [575] have been observed.”
Coronal loop oscillations Calculation of resonantly damped MHD quasi-mode kink oscillations of longitudinally stratified loops (2005, background): “Since then, several oscillating loops have been reported and thoroughly studied (Aschwanden et al. 2002; Schrijver et al. 2002; Nakariakov et al. 1999).”
Coronal loop oscillations - An interpretation in terms of resonant absorption of quasi-mode kink oscillations (2002, background): “New examples of coronal loop oscillations have been discovered in the TRACE data since then (Aschwanden et al. 2002; Schrijver et al. 2002).”
Standing Slow-Mode Waves in Hot Coronal Loops: Observations, Modeling, and Coronal Seismology (2010, background): “They were seen as spatial displacements with periods of 3−5 minutes and were apparently excited by flares or erupting filaments (Schrijver et al. 2002; Aschwanden et al. 2002).”
Hot coronal loop oscillations observed with SUMER: Examples and statistics (2003, background): “The loop oscillation cases detected by TRACE are relatively rare (in 6% of 255 flares inspected), and this rarity is consistent with the proposal that transverse oscillations are preferentially found on loops at or near separatrices (Schrijver et al. 2002).”
MHD seismology of coronal loops using the period and damping of quasi-mode kink oscillations (2007, background): “The statistics and derived physical properties of these events can be found in Aschwanden et al. (2002) and Schrijver et al. (2002).”
Coronal Seismology by Means of Kink Oscillation Overtones (2009, methodology): “…later, kink oscillations of coronal loops were first observed very accurately by the TRACE spacecraft (Transition Region And Coronal Explorer) (Schrijver et al. 1999, 2002; Aschwanden et al. 1999; Nakariakov et al. 1999; Aschwanden et al. 2002) (or Aschwanden et al. 2003, for an observational…”
Impulsive Phase Flare Energy Transport by Large-Scale Alfvén Waves and the Electron Acceleration Problem (2007, background): “De Pontieu et al. (2001) considered the damping by ion-neutral coupling in the lower chromosphere of large-scale coronal oscillations, observed in TRACE to be excited by flares and filament eruptions (Schrijver et al. 2002).”
Observational Tests of Damping by Resonant Absorption in Coronal Loop Oscillations (2003, background): “…a small subset of all active region loops exhibit oscillations after a global triggering event, e.g., during a flare or a filament destabilization (Schrijver et al. 2002), the mechanism of resonant absorption provides a plausible explanation that oscillations are most favored in loops with little…”
Coronal loop seismology using multiple transverse loop oscillation harmonics (2007, background): “Later on, oscillations in a sample of 17 loops were studied and analysed by Schrijver et al. (2002); Aschwanden et al. (2002).”