How to Channel Photospheric Oscillations into the Corona
By Bart De Pontieu, R. Erdélyi, I. Moortel. 2005
169 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/93b36e07335e1ad6e224915145c1bfe3c0e88f10
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
- Tongjiang Wang
- T. Van Doorsselaere
- Valery M. Nakariakov
- Giuseppe Nisticò
- Petr Jelínek
- D. Kolotkov
- R. Erdélyi
- Erwin Verwichte
In Molecular Biology
- Tongjiang Wang
- T. Van Doorsselaere
- Valery M. Nakariakov
- Giuseppe Nisticò
- R. Erdélyi
- Erwin Verwichte
- G. Verth
- Michael Ruderman
Citations in the corpus
- Standing Slow-Mode Waves in Hot Coronal Loops: Observations, Modeling, and Coronal Seismology (2010, background): “This close link between observed periodicity and location suggests that the waves are driven by the underlying p-modes oscillations (De Pontieu et al. 2005; De Moortel & Rosner 2007; Hindman & Jain 2008).”
- Magnetohydrodynamic Oscillations in the Solar Corona and Earth’s Magnetosphere: Towards Consolidated Understanding (2016, background): “In particular, De Pontieu et al. (2005) proposed that p-modes could reach coronal heights by nonlinear steepening of field-aligned acoustic waves in the case when the field is inclined away from the vertical.”