The damping of slow MHD waves in solar coronal magnetic fields
By I. Moortel, A. Hood. 2003
183 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/aef9ee63299ecc53100738cef1d601e3f3d2e6f7
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
- G. Verth
- Valery M. Nakariakov
- Giuseppe Nisticò
- D. Jess
- Petr Jelínek
- D. Kolotkov
In Molecular Biology
- Tongjiang Wang
- G. Verth
- T. Van Doorsselaere
- Valery M. Nakariakov
- Giuseppe Nisticò
- D. Jess
- R. Erdélyi
- Michael Ruderman
Citations in the corpus
- Standing Slow-Mode Waves in Hot Coronal Loops: Observations, Modeling, and Coronal Seismology (2010, background): “The rapid damping of these waves are mainly due to thermal conduction (De Moortel & Hood 2003; Klimchuk et al. 2004).”
- Magnetohydrodynamic Oscillations in the Solar Corona and Earth’s Magnetosphere: Towards Consolidated Understanding (2016, background): “The damping of these compressive waves is thought to be mainly due to classical dissipative processes (Ofman et al. 1999, 2000; Nakariakov et al. 2000), in particular thermal conduction (De Moortel and Hood 2003), and coronal loop/field line expansion (De Moortel and Hood 2004).”
- Multiwavelength Studies of MHD Waves in the Solar Chromosphere (2015, background): “…propagating magnetoacoustic waves with velocities in the range of 70–165 km s−1 and periodicities of 180–420 s (Ofman et al. 1999; Ofman and Wang 2002; De Moortel and Hood 2003, 2004; Mendoza-Briceño et al. 2004; Krishna Prasad et al. 2011, 2012a; Kobanov and Chelpanov 2014; Liu and Ofman 2014).”