Radiative equilibrium temperature profile is stable to convection.

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Consider the statement: 'Radiative equilibrium temperature profile is stable to convection.'

First, recall what radiative equilibrium means: the net radiative heating or cooling at each layer balances so that the temperature gradient is such that there is no net local energy gain or loss from radiation alone. This does not automatically guarantee stability against convection.

Schwarzschild criterion provides a way to assess convective stability. It states that a stratified layer becomes convectively unstable when the actual temperature gradient exceeds the adiabatic temperature gradient, i.e., when the radiative (or any) gradient is too steep compared with what a parcel would experience if displaced and adiabatically adjusted. In that case, a displaced parcel is warmer than its surroundings and continues to rise, driving convection.

Therefore, a radiative equilibrium profile can be convectively unstable if its radiative gradient is steeper than the adiabatic gradient. In many astrophysical and atmospheric contexts, a radiative zone that heats from the inside or above can develop a super-adiabatic gradient, triggering convection and disrupting a purely radiative profile.

Option analysis:
- If the statement claims stability to convection, that would be incorrect in cases where the radiative gradient is super-adiabatic. Such a profile is prone to overturning motions, mixing, and the onset of convection, so stability is not guaranteed.
- The logical flaw in the idea of universal stability is neglecting the dependence on the temperature gradient relative to the adiabatic gradient; stability is not an intrinsic property of 'radiative equilibrium' alone, but of the gradient comparison described by Schwarzschild.

In summary, the claim is not universally true because radiative equilibrium can still harbor convective instability when the radiative gradient exceeds the adiabatic gradient; therefore, the statement is false. Convection can modify a radiative equilibrium profile into a radiative-convective equilibrium, particularly in layers where heating is efficient or opacity causes steep gradients.

CLMTGR5001_002_2025_3 - Dynamics of Climate Variability and Chan PRACTICE QUIZ: Week 3 Lecture 3

Radiative equilibrium temperature profile is stable to convection.

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