Solar flux variation of the electron temperature morning overshoot in the equatorial F region
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چکیده
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Numerical Simulations of Penetration and Overshoot in the Sun
We present numerical simulations of convective overshoot in a twodimensional model of the solar equatorial plane. The simulated domain extends from 0.001 R⊙ to 0.93 R⊙, spanning both convective and radiative regions. We show that convective penetration leads to a slightly extended, mildly subadiabatic temperature gradient beneath the convection zone below which there is a rapid transition to a ...
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