Forecasting of the solar wind and geomagnetic storms with spacecraft at L1, L5 or trailing the Earth in its orbit

Grad-Shafranov reconstruction for interplanetary magnetic flux ropes

Calculates from knowledge of the solar wind plasma and magnetic field the Dst index

This repository provides a python code to infer morphological parameters of Coronal Mass Ejection using Cone model given by Xie et al.,2004.

https://ssc.shef.ac.uk

This project analyses space wether data of solar wind parameters and geomagnetic parameters, it establishes to observe the statistical relationships between all these parameters and highlights their behaviour during major space weather events such as solar flares and corona mass ejections that may subsequently result to geomagnetic storms.

This Repository contains all the work done during NIUS camp 14.2 under the guidance of Prof. Dipankar Banerjee and the allotted mentors Vaibhav Pant and Ritesh Patel

Classic time-elongation fitting for heliospheric imager data