For uniform composition, a stellar layer is convectively stable when ∇<∇ad and unstable when ∇>∇ad, where ∇=dlogT/dlogP.
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- Convection onset in a logarithmic-pressure grey atmosphere
- Convective instability of a square-root exponential atmospheric profile
- Dry adiabatic lapse rate
- Dry parcel buoyancy in a homogeneous atmosphere
- Grey-atmosphere convection onset with density-linear opacity
- Grey-atmosphere convection onset with eighth-power temperature opacity
- Grey-atmosphere convection onset with thirteenth-power opacity
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- Power-law opacity radiative envelope
- Radiative-envelope convection matching
- Stellar convective instability
- Stellar radiative temperature gradient
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