Nakariakov, VM, Tsiklauri, D, Kelly, A, Arber, TD and Aschwanden, MJ 2004, 'Acoustic oscillations in solar and stellar flaring loops' , Astronomy and Astrophysics, 414 (2) , L25-L28.
PDF (Publisher version)
Evolution of a coronal loop in response to an impulsive energy release is numerically modelled. It is shown that the loop density evolution curves exhibit quasi-periodic perturbations with the periods given approximately by the ratio of the loop length to the average sound speed, associated with the second standing harmonics of an acoustic wave. The density perturbations have a maximum near the loop apex. The corresponding field-aligned flows have a node near the apex. We suggest that the quasi-periodic pulsations with periods in the range 10-300 s, frequently observed in flaring coronal loops in the radio, visible light and X-ray bands, may be produced by the second standing harmonic of the acoustic mode.
|Uncontrolled Keywords:||Sun: flares, oscillations, corona, stars: flare, oscillations, coronae|
|Themes:||Subjects / Themes > Q Science > QB Astronomy
Subjects outside of the University Themes
|Schools:||Schools > School of Computing, Science and Engineering|
|Journal or Publication Title:||Astronomy and Astrophysics|
|Depositing User:||H Kenna|
|Date Deposited:||03 Sep 2007 14:20|
|Last Modified:||01 Dec 2015 00:02|
Actions (login required)
|Edit record (repository staff only)|