Structure, Evolution and Dynamics of Mesoscale and Synoptic Scale Convective Systems using the network of Doppler Weather Radar (DWR) and satellite observations.
Implementing Organization
Vikram Sarabhai Space Centre, ISRO, Trivandrum, Kerala
Principal Investigator
PI: Dr. K. N. Uma SPL
Vikram Sarabhai Space Centre, ISRO, Trivandrum, Kerala
VSSC
uma_kn@vssc.gov.in
CO-Principal Investigator
Dr. Radhika Ramachandran Space Physics Laboratory Vikram Sarabhai Space Centre
Kawdiar Thiruvananthapuram - 695003, INDIA
Indian Space Research Organisation PNRA-C27, Radhalayam, Sri Krishna Lane
CO-Principal Investigator
Dr. Siddarth Shankar Das
Vikram Sarabhai Space Centre, ISRO, Dept. of Space, Govt of India Thiruvananthapuram-695022, INDIA
Space Physics Laboratory
About
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
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