(19) Kato (20) extended Lighthill's theory to magnetohydrodynamic waves and found that Eq.
(1961) The heating of the solar chromosphere, plages, and corona by magnetohydrodynamic waves. Astrophys.
(2007) Coronal transverse magnetohydrodynamic waves in a solar prominence.
Zhelyazkov, "Magnetohydrodynamic waves and their stability status in solar spicules," Astronomy & Astrophysics, vol.
Mishonov, "Kelvin-Helmholtz instability of magnetohydrodynamic waves propagating on solar surges," Astrophysics and Space Science, vol.
Srivastava, "Can magnetohydrodynamic waves traveling on solar dark mottles become unstable?" Bulgarian Journal of Physics, vol.
This equation models Alfven waves and magnetohydrodynamic waves
in plasmas and also model subpicosecond or femtosecond pulses in single-mode optical fibers in nonlinear optics [11, 12].
Seventeen opening papers address eclipse-related issues of solar system physics, including eclipses and planetary transits, mass determination of small solar system bodies with ground-based observation, damping of magnetohydrodynamic waves
as a heating mechanism of solar corona, coronal heating and acceleration of the solar wind.
 studied the time damping of linear nonadiabatic magnetohydrodynamic waves in an unbounded plasma with coronal properties and found that behavior of the damping changes significantly when going from very small to very large wavenumbers and becomes almost constant for very large wavenumbers.
Ballester, "Time damping of linear non-adiabatic magnetohydrodynamic waves in an unbounded plasma with solar coronal properties," Astronomy and Astrophysics, vol.
Ballester, "Nonadiabatic magnetohydrodynamic waves in a cylindrical prominence thread with mass flow," Astrophysical Journal Letters, vol.