Influence of turbulent pressure on solar convective modes

Details Influence of turbulent pressure on solar convective modes Influence of turbulent pressure on solar convective modes

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.204..865a&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 204, Sept. 1983, p. 865-881.

Astronomy and Astrophysics

Astronomy

6

Convective Flow, Plasma Turbulence, Pressure Effects, Solar Granulation, Mixing Length Flow Theory, Propagation Modes, Solar Atmosphere, Stellar Envelopes, Stellar Models

Scientific paper

The stability of linear convective modes in the solar envelope model is investigated by incorporating in a very crude manner the effects of turbulent pressure and eddy transport coefficients calculated in the mixing length approximation. It is demonstrated that for a reasonable choice of the parameters there occur two peaks in the growth rate versus horizontal wavenumber plot which correspond to the observed features associated with granulation and supergranulation.

Affiliated with

Also associated with

No associations

Rating

Influence of turbulent pressure on solar convective modes 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 Influence of turbulent pressure on solar convective modes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Influence of turbulent pressure on solar convective modes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1593181