• Corpus ID: 117443092

Effect of the steady flow on spatial damping of small-amplitude prominence oscillations

@article{Singh2007EffectOT,
  title={Effect of the steady flow on spatial damping of small-amplitude prominence oscillations},
  author={Kadira Analisa Singh and R{\'o}bert Erd{\'e}lyi and Bhola N. Dwivedi},
  journal={arXiv: Astrophysics},
  year={2007}
}
Aims. Taking account of steady flow in solar prominences, we study its effects on spatial damping of small-amplitude non-adiabatic magnetoacoustic waves in a homogeneous, isothermal, and unbounded prominence plasma. Methods. We model the typical feature of observed damped oscillatory motion in prominences, removing the adiabaticity assumption through thermal conduction, radiation and heating. Invoking steady flow in MHD equations, we linearise them under small-amplitude approximation and obtain… 
1 Citations
Effect of steady flow and Newton's cooling on the propagation and damping of small-amplitude prominence plasma oscillations
Abstract We study the propagation and damping of small-amplitude prominence oscillations invoking steady flow and radiative losses due to Newton's cooling with constant relaxation time. We find that

References

Dynamics and Structure of Quiescent Solar Prominences
1 Introduction to Quiescent Solar Prominences (E R Priest).- 1.1 Basic Description.- 1.1.1 Different Types.- 1.1.2 Properties.- 1.1.3 Development.- 1.1.4 Structure.- 1.1.5 Eruption.- 1.2 Basic