Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...241..625u&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 241, no. 2, Jan. 1991, p. 625-634.
Astronomy and Astrophysics
Astrophysics
62
Longitudinal Waves, Magnetic Flux, Solar Atmosphere, Transverse Waves, Wave Propagation, Adiabatic Conditions, Boundary Conditions, Magnetic Resonance, Plasma Waves, Solar Magnetic Field, Time Dependence
Scientific paper
The nonlinear time-dependent response to purely transverse foot point shaking of a vertical magnetic flux tube in the solar atmosphere was studied. The adiabatic calculations show the generation of a longitudinal wave mode which has twice the frequency of the transverse wave. The amplitude of the longitudinal wave increases with the wave period and with the magnitude of the shaking. Due to the action of centrifugal forces significant lifting of the tube gas was found. A forced oscillator type resonance occurs which depends on the tube length.
Musielak Zdzislaw E.
Ulmschneider Peter
Zaehringer K.
No associations
LandOfFree
Propagation of nonlinear longitudinal-transverse waves along magnetic flux tubes in the solar atmosphere. I - Adiabatic waves 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 Propagation of nonlinear longitudinal-transverse waves along magnetic flux tubes in the solar atmosphere. I - Adiabatic waves, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Propagation of nonlinear longitudinal-transverse waves along magnetic flux tubes in the solar atmosphere. I - Adiabatic waves will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1894626