A Graphical Method for Estimating Overshoot in Convective Stellar Atmospheres

Details A Graphical Method for Estimating Overshoot in Convective Stellar Atmospheres A Graphical Method for Estimating Overshoot in Convective Stellar Atmospheres

Apr 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974ap%26ss..27..303c&link_type=abstract

Astrophysics and Space Science, Volume 27, Issue 2, pp.303-305

Astronomy and Astrophysics

Astrophysics

Scientific paper

A graphical method for estimating convective overshoot in stellar
atmospheres is proposed. Applying the method to the solar atmosphere, we
find that a convective element which starts at a depth of about 1000 km
below the top of convection zone can penetrate to a height about 300 km
above it.

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