On the problem of f-mode generation in the solar atmosphere

Details On the problem of f-mode generation in the solar atmosphere On the problem of f-mode generation in the solar atmosphere

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..132..205z&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 132, April 1991, p. 205-213.

Physics

2

Helioseismology, Solar Atmosphere, Solar Oscillations, Wave Excitation, Hydrodynamic Equations, Nonadiabatic Conditions, Wave Equations

Scientific paper

The theory of nonadiabatic high-l f-mode is developed. It is proved that high-l f-modes cannot be excited or damped by any nonadiabatic mechanism including k- and gamma-mechanisms, radiative and convective Cowling mechanisms, and the epsilon-mechanism. Solar 5-min high-l f-modes can be excited only by a nonlinear interaction with convection of p-modes. The seismology of the solar atmosphere on the basis of 5-min f-mode observations is considered.

Affiliated with

Also associated with

No associations

Rating

On the problem of f-mode generation in the solar atmosphere 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 On the problem of f-mode generation in the solar atmosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the problem of f-mode generation in the solar atmosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1794471