Damping of Coronal Loop Oscillations: Calculation of Resonantly Damped Kink Oscillations of One-dimensional Nonuniform Loops
By T. Van Doorsselaere, Jesse Andries, Stefaan Poedts, M. Goossens. 2004
165 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/c92c83d0391a852c66a81ba84b873032681c0dc3
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In Astronomy and Astrophysics
- R. Erdélyi
- Tongjiang Wang
- T. Van Doorsselaere
- Valery M. Nakariakov
- Erwin Verwichte
- Michael Ruderman
- Jesse Andries
- G. Verth
In Molecular Biology
- R. Erdélyi
- Tongjiang Wang
- T. Van Doorsselaere
- Valery M. Nakariakov
- Michael Ruderman
- Erwin Verwichte
- G. Verth
- Jesse Andries
Citations in the corpus
- MHD seismology of coronal loops using the period and damping of quasi-mode kink oscillations (2007, methodology): “As shown by Van Doorsselaere et al. (2004), these differences increase for large inhomogeneity length-scales and high damping rates.”
- Standing Slow-Mode Waves in Hot Coronal Loops: Observations, Modeling, and Coronal Seismology (2010, background): “…been proposed to explain the rapid decay of transverse oscillations observed by TRACE, among which resonant absorption (Ruderman & Roberts 2002; Van Doorsselaere et al. 2004; Goossens 2008), phase mixing (Nakariakov et al. 1999; Ofman & Aschwanden 2002), and lateral wave leakage (Brady & Arber…”
- Coronal loop oscillations Calculation of resonantly damped MHD quasi-mode kink oscillations of longitudinally stratified loops (2005, background): “Eigenmodes of such highly inhomogeneous loop models have been calculated recently by Van Doorsselaere et al. (2004a).”
- CORONAL LOOP OSCILLATIONS OBSERVED WITH ATMOSPHERIC IMAGING ASSEMBLY—KINK MODE WITH CROSS-SECTIONAL AND DENSITY OSCILLATIONS (2011, methodology): “We acknowledge constructive and helpful discussions with Valery Nakariakov, Erwin Verwichte, Jaume Terradas, Robertus Erdelyi, Richard Morton, Leon Ofman, Tom Van Doorsselaere, Ineke De Moortel, Mag Selwa, Michael Ruderman, and James McAteer, mostly during a meeting on “Coronal Heating and Waves” sp”
- Coronal Waves and Oscillations (2005, background): “Recently, Verwichte et al. (2005) presented for the first time a direct observational study of propagating fast waves in an open magnetic structure, i.”
- Transverse Oscillations of Coronal Loops (2009, methodology): “This observation inspired Van Doorsselaere et al. (2004a) to study the damping of kink 26 oscillations of magnetic flux tubes numerically.”
- Hinode observations of transverse waves with flows in coronal loops (2008, background): “There are three main classes of wave damping mechanism that are currently debated in the literature (e.g., Roberts 2000; Ruderman & Roberts 2002; Ofman 2002; Ofman & Aschwanden 2002; Goossens et al. 2002; Van Doorsselaere et al. 2004; Aschwanden 2005): leakage, resonant absorption or mode conversion”
- Effect of longitudinal magnetic and density inhomogeneity on transversal coronal loop oscillations (2008, background): “Applying this theory to TRACE data of loop oscillations, attempts have been made to estimate coronal density scale heights (see e.g., Andries et al. 2005a; Van Doorsselaere et al. 2007).”
- Coronal loop seismology using multiple transverse loop oscillation harmonics (2007, methodology): “Early analytical work on this mechanism was done by Goossens et al. (1995); Ruderman & Roberts (2002) and numerical modelling was done by Van Doorsselaere et al. (2004a) to extend the standard loop model to radially inhomogeneous loops.”
- Magnetohydrodynamic Oscillations in the Solar Corona and Earth’s Magnetosphere: Towards Consolidated Understanding (2016, methodology): “This formula was numerically checked for larger l/a with an eigenvalue code by Van Doorsselaere et al. (2004a), who found deviations limited to 25 % for the damping time for a broad”
- On the nature of kink MHD waves in magnetic flux tubes (2009, methodology): “Subsequently Van Doorsselaere et al. (2008)argued strongly against the possible presence of Alfvén waves in the solar corona emphasising that Alfvén waves cannot be but torsional.”