Interplanetary parameters and their correlation with geomagnetic storms

It has been established that the main cause of the geomagnetic storm is believed a large Interplanetary Magnetic Field (IMF) structure which has an intense and long duration southward magnetic field component. The previous study suggests that the strength of geomagnetic storm is strongly dependent on the total magnetic field B total. They interact with Earth’s magnetic field and facilitate the transport of energy into the Earth’s atmosphere by reconnection process. Present paper shows the study of the Interplanetary Magnetic Field (IMF) parameters during geomagnetic storms. We have studied more than 200 geomagnetic storms weighed by disturbance storm time (Dst) <-50 nT, observed during the year of 2007 to 2016.