Principles of Magnetohydrodynamics
By Stefaan Poedts. 2004
168 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/e601dc0909f319b733482011f357710cd919dda7
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
- T. Van Doorsselaere
- Erwin Verwichte
- Tongjiang Wang
- G. Verth
- Jesse Andries
- Valery M. Nakariakov
- Iñigo Arregui
In Molecular Biology
- R. Erdélyi
- T. Van Doorsselaere
- Erwin Verwichte
- G. Verth
- Jesse Andries
- Tongjiang Wang
- L. Ofman
- Iñigo Arregui
Citations in the corpus
- Multiwavelength Studies of MHD Waves in the Solar Chromosphere (2015, background): “The phase speeds of these waves are well ordered: 0 ≤ vslow ≤ vA ≤ vf ast , and also their velocities are mutually perpendicular, vslow ⊥ vA ⊥ vf ast (Goedbloed and Poedts 2004).”
- Coronal Seismology by Means of Kink Oscillation Overtones (2009, background): “3.2), which is just a specific form of the Rayleigh-Ritz variational principle where the normal mode frequencies are found as stationary values of the Rayleigh quotient representing the ratio between the wave potential energy and wave inertia (e.g., Goedbloed and Poedts 2004, Sect.”
- Magnetic field inclination and atmospheric oscillations above solar active regions (2006, methodology): “In the MHD context, we would like Da to represent the ‘acoustic wave’ and Db the ‘magnetic wave’, with η quantifying the mode transmission (fast-to-slow or vice versa), which occurs in the neighbourhood of the ‘star points’ Da = Db = 0.”
- Magnetohydrodynamic waves in solar partially ionized plasmas: two-fluid approach (2011, unknown): “The fluid equations for each species can be derived from Boltzmann kinetic equations, which have the forms (Braginskii 1965; Goedbloed & Poedts 2004) ∂ne ∂t + ∇ · (neVe) = 0, (1) ∂ni ∂t + ∇ · (niVi) = 0, (2) ∂nn ∂t + ∇ · (nnVn) = 0, (3) mene ( ∂Ve ∂t + (Ve · ∇)Ve ) = −∇pe − ∇ · πe −ene ( E + 1 c Ve…”
- Coronal Heating by MHD Waves (2020, background): “An extensive body of literature on both resonant absorption and phase mixing exist, for which we refer the interested reader to reviews by e.g. Aschwanden (2004), Goedbloed and Poedts (2004), Goossens et al. (2011).”