Comparative planetary heat transport and observed phase curves
Research context
research method · conditional · As of 2026-10-10
Planetary circulation couples radiation and dynamics; comparing advective, radiative and rotation time scales organizes possible regimes.
Key knowledge
Planetary circulation couples radiation and dynamics; comparing advective, radiative and rotation time scales organizes possible regimes. Timescale estimates give qualitative guidance, while measured phase curves also depend on vertical contribution functions, composition and clouds.
Values and equations
τ_adv≈L/U
- τ_adv
- Horizontal advective timescale s
- L
- Declared horizontal transport distance m
- U
- Characteristic velocity m s^-1
Conditions and scope
- Use shared gravity, radius, pressure, EOS and irradiation conventions across planets.
- A phase offset alone does not uniquely measure wind speed or interior heat; use a coupled forward observation model.
Sources · 2
References
Sources retain their recorded scope. A source link alone does not establish verification of every statement.
Evidence and review
Atmospheric Circulation of Exoplanets: Sections 2–3 and 5: thermodynamic equation, radiative/advective times and comparative circulation (selected source body inspected). MESA equation-of-state module: Blended EOS domains, thermodynamic derivatives and composition assumptions (selected source body inspected).
2026-10-10 · Bounded source check of the recorded statement and conditions. This does not certify a unique physical model, reproduce the cited study or replace independent branch review.
Entry details
Permanent link to this entry ↗- Record identity
- research-earth-planet-redistribution
- Revision
- research.1
- Structured reference record
- Postgraduate & research reference