Abstract
The effects of longwave radiation on tropical cyclone intensification, with an emphasis on the mature stage, are explored in an idealized modeling framework. Results show that although the cloud-radiative effect aids in early intensification of the vortex, it does not promote increase in the maximum tangential wind (Vmax) and could even reduce Vmax at the mature stage. At later stages, maximum radiative heating is located outside the eyewall and promotes convection there, and the secondary circulation encourages convergence of absolute angular momentum outside the eyewall instead of near the eyewall region, based on a budget analysis. Clear-sky radiative cooling helps invigorate domainwide convection, also limiting the Vmax increase at later stages. The area-averaged frozen moist static energy (FMSE) variance increases even though Vmax decreases. In this sense, the FMSE variance is similar to the monotonically growing integrated kinetic energy, and is more indicative of the system-scale strength than of Vmax. Sensitivity experiments are performed with random initial perturbations and varied initial soundings. An axisymmetric model with a 10-member ensemble not only confirms the results from three-dimensional simulations, but also demonstrates that the weak radiative heating outside the eyewall is indeed able to slow down Vmax within 1 day.
| Original language | English |
|---|---|
| Pages (from-to) | 1829-1845 |
| Number of pages | 17 |
| Journal | Journal of the Atmospheric Sciences |
| Volume | 80 |
| Issue number | 7 |
| DOIs | |
| Publication status | Published - Jul 2023 |
UN SDGs
This output contributes to the following UN Sustainable Development Goals (SDGs)
-
SDG 3 Good Health and Well-being
Keywords
- Cloud resolving models
- Mesoscale models
- Tropical cyclones
Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver