Solar p-mode eigenfrequencies are decreased by turbulent convection

Details Solar p-mode eigenfrequencies are decreased by turbulent convection Solar p-mode eigenfrequencies are decreased by turbulent convection

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984sci...226..687b&link_type=abstract

Science (ISSN 0036-8075), vol. 226, Nov. 9, 1984, p. 687-689.

Astronomy and Astrophysics

Astrophysics

42

Astrophysics, Solar Oscillations, Stellar Models, Convection, Stellar Structure, Turbulent Flow, Wave Fronts, Wave Propagation

Scientific paper

Average solar p-mode eigenfrequencies are decreased by large fluctuating velocity fields in the upper convection zone. This effect is greatest for modes with large horizontal wave numbers and frequencies. It is large enough to affect estimates of the depth of the convection zone and may carry useful information about the structure of solar convective turbulence.

Affiliated with

Also associated with

No associations

Rating

Solar p-mode eigenfrequencies are decreased by turbulent convection 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 Solar p-mode eigenfrequencies are decreased by turbulent convection, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar p-mode eigenfrequencies are decreased by turbulent convection will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1757119