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Structure, Evolution and Dynamics of Mesoscale and Synoptic Scale Convective Systems using the network of Doppler Weather Radar (DWR) and satellite observations.

Implementing Organization

Principal Investigator
PI: Dr. K. N. Uma SPL
VSSC, Trivandrum, Kerala
uma_kn@vssc.gov.in
CO-Principal Investigator
Dr. Radhika Ramachandran Space Physics Laboratory Vikram Sarabhai Space Centre
Indian Space Research Organisation PNRA-C27, Radhalayam, Sri Krishna Lane, Kawdiar Thiruvananthapuram - 695003, INDIA, Dr. Siddarth Shankar Das, Space Physics Laboratory, Vikram Sarabhai Space Centre, ISRO, Dept. of Space, Govt of India Thiruvananthapuram-695022, INDIA

Project Overview

It is proposed to identify convective storms using Thunderstorm Identification, Tracking, and Analysis and Nowcasting (TITAN) algorithm and represent in terms of duration, area, volume, propagation speed and direction; echo top height, etc.. In addition to the above, as mentioned in the objectives, using multiple radars, the mosaic of radar reflectivity over the Indian region will be brought out
Funding Organization
Quick Information
Area of Research
Earth, Atmosphere & Environment Sciences
Focus Area
Atmospheric Science
Start Date
2023
Status
ongoing
Output
No. of Research Paper
00
Technologies (If Any)
00
No. of PhD Produced
00
Publications
00
No. of Patents
Filed : 00
Grant : 00
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