Determination of the Coronal Density Stratification from the Observation of Harmonic Coronal Loop Oscillations

By Jesse Andries, Iñigo Arregui, M. Goossens. 2005

209 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/22a66708a1f247acdb852fac43bbd53bc9d738bd

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

1. R. Erdélyi
2. Tongjiang Wang
3. T. Van Doorsselaere
4. Valery M. Nakariakov
5. Erwin Verwichte
6. Michael Ruderman
7. G. Verth
8. Jesse Andries

In Molecular Biology

1. R. Erdélyi
2. Tongjiang Wang
3. T. Van Doorsselaere
4. Valery M. Nakariakov
5. Michael Ruderman
6. Erwin Verwichte
7. Jesse Andries
8. G. Verth

Citations in the corpus

• Coronal loop seismology using multiple transverse loop oscillation harmonics (2007, methodology): “Using the model of Andries et al. (2005a), we find L/πH = 1.02+0.46−0.44.”
• Effect of longitudinal magnetic and density inhomogeneity on transversal coronal loop oscillations (2008, methodology): “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).”
• Standing Slow-Mode Waves in Hot Coronal Loops: Observations, Modeling, and Coronal Seismology (2010, background): “…field (Nakariakov & Ofman 2001; Aschwanden et al. 2002; Wang et al. 2007), energy transport coefficients (Nakariakov et al. 1999; Ofman & Aschwanden 2002), density stratification (e.g. Andries et al. 2005; Van Doorsselaere et al. 2008a), and loop temperature (Marsh et al. 2009; Wang et al. 2009b).”
• Decayless low-amplitude kink oscillations: a common phenomenon in the solar corona? (2015, methodology): “In particular, kink oscillations are used for estimating coronal magnetic field (e.g. Nakariakov & Ofman 2001), density stratification (e.g. Andries et al. 2005; Van Doorsselaere et al. 2008), the variation of the magnetic field along the loop (e.g. Ruderman et al. 2008; Verth & Erdélyi 2008), and…”
• Transverse Oscillations of Coronal Loops (2009, methodology): “…eigenfrequencies, ωe0n = πCk(2n − 1)/2L and ωo0n = πCkn/L. Dymova and Ruderman (2006a) also carried out the calculations of eigenfrequencies for the same dependence of the density on z as that used by Andries et al. (2005b) and compared their results with those obtained by Andries et al. (2005b).”
• MHD seismology of coronal loops using the period and damping of quasi-mode kink oscillations (2007, methodology): “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, based on calculations of Andries et al. 2005b) to determine the density stratification in those loops.”
• 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).”