MHD seismology of coronal loops using the period and damping of quasi-mode kink oscillations
By Iñigo Arregui, Jesse Andries, T. Van Doorsselaere, M. Goossens, Stefaan Poedts. 2007
137 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/74c7e34f42a4e33d8b088b19c770c7c824093574
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- R. Erdélyi
- Tongjiang Wang
- T. Van Doorsselaere
- Valery M. Nakariakov
- Erwin Verwichte
- G. Verth
- Jesse Andries
- M. Goossens
In Molecular Biology
- R. Erdélyi
- Tongjiang Wang
- T. Van Doorsselaere
- Valery M. Nakariakov
- Erwin Verwichte
- G. Verth
- Jesse Andries
- Giuseppe Nisticò
Citations in the corpus
- Hinode observations of transverse waves with flows in coronal loops (2008, background): “…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; Ballai 2007; Arregui et al. 2007).”
- On the nature of kink MHD waves in magnetic flux tubes (2009, background): “This is clearly illustrated in a recent analytical seismological study by Goossens et al. (2008) which complemented a fully numerical seismology investigation by Arregui et al. (2007).”
- Coronal loop seismology using multiple transverse loop oscillation harmonics (2007, background): “Verwichte et al. (2006b) determined the radial density structure in oscillation coronal loops, and Arregui et al. (2007) found a lower bound for the internal Alfvén transit time.”
- Magnetohydrodynamic Oscillations in the Solar Corona and Earth’s Magnetosphere: Towards Consolidated Understanding (2016, background): “Both the period and damping time can be directly observed, and the combination of the information in them with numerical and analytical modelling, has been used by Arregui et al. (2007).”
- Effect of longitudinal magnetic and density inhomogeneity on transversal coronal loop oscillations (2008, background): “…from the work of Hollweg & Yang (1988), it has been shown that varying plasma density in the radial direction results in a change of period and damping of MHD waves (see e.g., Ruderman & Roberts 2002; Goossens et al. 2002; Aschwanden et al. 2003; Van Doorsselaere et al. 2004; Arregui et al. 2007).”