Vertical oscillations of a coronal loop observed by TRACE

By Tongjiang Wang, S. Solanki. 2004

146 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/fd23448728e48eeda104ce5cda18db5e132009c9

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. Tongjiang Wang
2. R. Erdélyi
3. T. Van Doorsselaere
4. Valery M. Nakariakov
5. Erwin Verwichte
6. Michael Ruderman
7. L. Ofman
8. Markus J. Aschwanden

In Molecular Biology

1. Tongjiang Wang
2. R. Erdélyi
3. Valery M. Nakariakov
4. T. Van Doorsselaere
5. Erwin Verwichte
6. Michael Ruderman
7. L. Ofman
8. Giuseppe Nisticò

Citations in the corpus

• Standing Slow-Mode Waves in Hot Coronal Loops: Observations, Modeling, and Coronal Seismology (2010, methodology): “A fundamental vertically polarized kink mode oscillation was first identified by Wang & Solanki (2004) using TRACE observations, and a fundamental horizontally polarized kink mode was recently identified by Verwichte et al. (2009) using STEREO/EUVI.”
• Coronal loop seismology using multiple transverse loop oscillation harmonics (2007, background): “Wang & Solanki (2004) found oscillations with a vertical polarisation, and Li & Gan (2006) observed oscillations in shrinking loops.”
• Magnetohydrodynamic Oscillations in the Solar Corona and Earth’s Magnetosphere: Towards Consolidated Understanding (2016, result): “This result is consistent with observations, as vertical kink oscillations (e.g. Wang and Solanki 2004; White et al. 2012; Kim et al. 2014) have been detected much more rarely than horizontal.”
• The FIP and Inverse FIP Effects in Solar and Stellar Coronae (2015, background): “Such wave motions observed in the solar corona have been identified as kink (a subset of fast mode) mode waves (e.g., Nakariakov et al., 1999; Wang and Solanki, 2004).”
• Hinode observations of transverse waves with flows in coronal loops (2008, methodology): “Since the observations are near the solar limb and the threads are seen to be displaced in the vertical direction in the plane of the sky, it is likely that the oscillations contain a vertical component, similar to the vertical oscillations recently observed by TRACE (Wang & Solanki 2004).”
• CORONAL LOOP OSCILLATIONS OBSERVED WITH ATMOSPHERIC IMAGING ASSEMBLY—KINK MODE WITH CROSS-SECTIONAL AND DENSITY OSCILLATIONS (2011, background): “This characteristic seems to be a particular property of oscillations in the loop plane (Figure 7), also called “vertical polarization of kink mode” (Wang & Solanki 2004; Verwichte et al. 2006a, 2006b), which would not occur (to first order) for transverse oscillations in the direction…”
• Transverse Oscillations of Coronal Loops (2009, background): “However Wang and Solanki (2004) reported the observations by TRACE of the vertically polarised oscillations of coronal loops (see also Wang et al. (2008)).”