Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005a%26a...430.1109a&link_type=abstract
Astronomy and Astrophysics, v.430, p.1109-1118 (2005)
Astronomy and Astrophysics
Astrophysics
97
Sun: Corona, Sun: Magnetic Fields, Sun: Oscillations
Scientific paper
The observed coronal loop oscillations and their damping are often theoretically described by the use of a very simple coronal loop model, viz. a straight, longitudinally invariant, axi-symmetric, and pressureless flux tube with a different density inside and outside of the loop. In this paper we generalize the model by including longitudinal density stratification and we examine how the longitudinal density stratification alters the linear eigenmodes of the system, their oscillation frequencies, and the damping rates by resonant absorption.
Appendix A is only available in electronic form at http://www.edpsciences.org
Andries Jesse
Arregui Inigo
Doorsselaere Tom Van
Goossens Marcel
Hollweg Joseph V.
No associations
LandOfFree
Coronal loop oscillations. Calculation of resonantly damped MHD quasi-mode kink oscillations of longitudinally stratified loops does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Coronal loop oscillations. Calculation of resonantly damped MHD quasi-mode kink oscillations of longitudinally stratified loops, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Coronal loop oscillations. Calculation of resonantly damped MHD quasi-mode kink oscillations of longitudinally stratified loops will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1744823