EGU21-12128
https://doi.org/10.5194/egusphere-egu21-12128
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Kinetic energy generation in cross-equatorial flow and the Somali Jet

Ashwin K Seshadri1 and Vishal Dixit2
Ashwin K Seshadri and Vishal Dixit
  • 1Centre for Atmospheric and Oceanic Sciences and Divecha Centre for Climate Change, Indian Institute of Science, Bangalore, India (ashwins@iisc.ac.in)
  • 2Department of Remote sensing and Geosciences, TU Delft, Netherlands (v2dixit@gmail.com)
In response to the north-south pressure gradients set by the annual march of the Sun, a cross-equatorial flow that turns to become a low-level zonal jet at around 10 ° N (also known as Somali jet) is set in the lower troposphere (around 850 hPa) over the Indian ocean. These flows play a fundamental role in the Indian monsoon. A detailed understanding of small and large scale drivers of this flow is lacking. Here we present the analysis of Kinetic Energy (KE) budget of the low level flow using high spatio-temporal resolution ERA5 reanalysis to identify sources and sinks of KE generation. We find that a significant KE generation occurs over East African highlands, Western Ghats and the Arabian sea. Over the oceans, the KE generation occurs mainly due to cross-isobaric meridional winds in the boundary layer. In contrast, over East African highlands and Western ghats KE generation maximizes just above the boundary layer and mainly occurs due to interaction of flow with the orography. We propose a simple model to decompose lower tropospheric KE generation into contributions from surface pressure, orography and free-tropospheric gradients.

How to cite: Seshadri, A. K. and Dixit, V.: Kinetic energy generation in cross-equatorial flow and the Somali Jet, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-12128, https://doi.org/10.5194/egusphere-egu21-12128, 2021.

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