Abstract:
The Southern Ocean (SO) marine atmospheric boundary layer (MABL), regulated by continuous air-sea exchanges, plays a key role in transporting exchanges between tropics and poles. Among SO sectors, the Indian Ocean sector of SO (ISSO) remained least explored in terms of MABL characterization and is examined in this study. In ISSO, occurrence of sharp oceanic thermohaline fronts regulates the vertical thermodynamic structure of MABL, clouds, and inversions. In this study, these properties of ISSO MABL are investigated over three oceanic domains (Sub-Tropical Indian Ocean (STIO), ISSO, and High-Latitude SO (HLSO)). To achieve this, near-sea surface air-sea exchanges along with profiles of meteorological parameters generated between 25°S and 68°S and 57°E to78°E during three field campaigns conducted in the austral summers of 2017, 2018, and 2020 were utilized. Results showed strong SST-Tair variability across the study region. In STIO, positive SST-T sub(air) indicated Low-Level Cold Air Advection (LLCAA)-induced destabilized and coupled MABLs capped by multiple inversions (>3INV's of strength approximately 0.35 K m sup(-1) above approximately 1200 m) and thin mid/high-altitudes clouds (cloud-base approximately 830 m, cloud-top approximately 2309 m, and cloud-thickness approximately 758 m). Over ISSO and northern HLSO, weak and negative SST-T sub(air) indicated Low-Level Warm Air Advection (LLWAA)-induced stratified and decoupled MABLs. Aided by advective mixing of multiple air-masses, low-level thick multilayered clouds (>2 layers, average cloud-base approximately 604 m, cloud-top approximately 2288 m, and cloud-thickness approximately 1314 m) and multiple strong high-level inversions (>2INV's, strength>0.4 K m sup(-1), approximately 1836 m) was observed. In HLSO, weakly positive SST-T sub(air) indicated LLCAA-induced weakly destabilized MABLs capped by mid-altitude inversions (strength approximately 0.22 K m sup(-1), approximately 1632 m) and mid-altitude clouds (cloud-base approximately 979 m, cloud-top approximately 2465 m, and cloud-thickness approximately 1263 m) supported by sublimation leading to virga conditions.
