Guide:
The project aims to study the velocity profile of the meridional flow on the solar surface by analysing the evolution of the magnetic field.
Guide: Dr. Bidya Binay Karak (IIT BHU)
To answer this question, we have performed a set of simulations using Babcock-Leighton type dynamo models at different values of dynamo supercriticality and analysed the various magnetic cycle features.
Guide: Dr. Bidya Binay Karak (IIT BHU)
The primary focus of our investigation revolved around understanding the impact of the supercriticality of the solar dynamo on the prediction of the solar cycle and the prediction of the strength of the 25th solar cycle
Guide: Dr. Shravan Hanasoge
This project focused on building the pipeline to detect l = 3 modes in Red Giants.