We find that BL values are close to zero within both the TC interior and its environment (the TC interior has a slightly larger BL), implying that TCs are in a state of convective quasi-equilibrium (QE). However, this state of QE is attained through different pathways within the storm interior and its environment. The storm interior has lower CAPEL values than its environment at higher intensities. This is because the TC’s warm core strengthens the vertical stratification, plausibly due to subsidence within the TC eye. Quantitatively this is shown using equivalent potential temperature (θe) variations. Both the boundary layer averaged θe (θeB) and the lower-tropospheric saturated θe (θeLsat) increase as one moves from the TC environment to its interior, but θeLsat increases faster than θeB with intensity. The storm interior is also more moist than its environment in the lower troposphere (smaller SUBSATL values; closer to saturation), with average θe in the lower-free troposphere (θeL) increasing faster than θeLsat as one moves from the storm environment to its interior. The high moisture-low CAPEL values with the TC interior, and the relatively low moisture-high CAPEL values in the TC environment thus enforce a state of near-zero BL, both within and outside the storm. We also found that TCs with higher intensity had lower SUBSATL values in their interior, relative to their environment.

