Investigation of three events of solar parameters and Interplanetary Coronal Mass ejections during the maximum phase of solar cycle 24

Abstract

This paper analyzes the Three events of Solar Parameters and Interplanetary Coronal Mass Ejections in the maximum phase of Solar Cycle 24 and focuses on the magnetic activity of interplanetary coronal mass ejection during the solar cycle 24. We investigate the magnetic field magnitude (B), Proton temperature (Tp), Proton density (Np). From this study, we find the highest peak of IP (Interplanetary) shocks on disk center MC (Magnetic cloud) events during the solar cycle 24 and also we investigate the magnetic activity of the solar cycle. In this study, we find that the ACE spacecraft shows the fastest coronal mass ejection and highest interplanetary shock wave on solar cycle 24. It is important to note that extreme events can happen at any time during a cycle. In solar cycle 24, from July 13, 2012 to July 15, 2012 largest storm occurred because the magnetic field was -52nT and linear speed was 1500 km s$^{-1}$ observed.