Observational study of interplanetary coronal mass ejections and flare in the solar corona

Interplanetary Coronal Mass Ejections (ICMEs) are the region of light scattered due to the electron densities in solar corona. The main objective of the study is to determine the distributions of Coronal Mass Ejections (CMEs) and solar flare parameters for the purpose of establishing the relationship between CME/flare properties derived from remote solar observations at the Earth. The identified CMEs are measured and their basic attributes are catalogued in a data base known as the SOHO/LASCO CME catalog. We have investigated some properties of all the fast and slow CMEs events. Our results reflect some of relatively well-known relationships between remotely observed solar properties, namely the importance of CME linear speed, angular width and associated solar flare. We also utilized various types of CME associated with different times of the solar cycle to estimate the impact on Earth. This paper presents the possible interpretations of the global CMEs and solar flare parameters, the summary of results obtained using the extensive events of Solar Energetic Particles (SEP) and radio burst at low frequency range associated with the energetic CME are greatly discussed.