International Journal of Astronomy and Astrophysics, 2019, 9, 191-199 http://www.scirp.org/journal/ijaa ISSN Online: 2161-4725 ISSN Print: 2161-4717 DOI: 10.4236/ijaa.2019.93014 Aug. 30, 2019 191 International Journal of Astronomy and Astrophysics The Analysis of Interplanetary Shocks Associated with Six Major Geo-Effective Coronal Mass Ejections during Solar Cycle 24 Shirsh Lata Soni 1* , Prithvi Raj Singh 2 , Bharti Nigam 1 , Radhe Syam Gupta 1 , Pankaj Kumar Shrivastava 3 1 Department of Physics, Govt. P.G. College, Satna, India 2 Department of Physics, APS University, Rewa, India 3 Department of Physics, Govt. P.G. Model Science College, Rewa, India Abstract A Coronal Mass Ejection (CME) is an ejection of energetic plasma with magnetic field from the Sun. In traversing the Sun-Earth distance, the ki- nematics of the CME is immensely important for the prediction of space weather. The objective of the present work is to study the propagation properties of six major geo-effective CMEs and their associated interplaneta- ry shocks which were observed during solar cycle 24. These reported CME events produced intense geo-magnetic storms (Dst > 140 nT). The six CME events have a broad range of initial linear speeds ~600 - 2700 km/sec in the LASCO/SOHO field of view, comparing two slow CMEs (speed ~579 km/sec and 719 km/sec), three moderate speed CMEs (speed ~1366, 1571, 1008 km/sec), and one fast CME (speed ~2684 km/sec). The actual arrival time of the reported events is compared with the arrival time calculated using the Empirical Shock Arrival model (ESA model). For acceleration estimation, we utilize three different acceleration-speed equations reported in the previous literatures for different acceleration cessation distance (ACD). In addition, we compared the transit time estimated using the second-order speed of CMEs with observed transit time. We also compared the observed transit time with transit time obtained from various shock arrival model. From our present study, we found the importance of acceleration cessation distance for CME propagation in interplanetary space and better acceleration speed for transit time calculation than other equations for CME forecasting. Keywords Coronal Mass Ejection (CME), IP Shock, Geomagnetic Strom How to cite this paper: Soni, S.L., Singh, P.R., Nigam, B., Gupta, R.S. and Shrivasta- va, P.K. (2019) The Analysis of Interplane- tary Shocks Associated with Six Major Geo-Effective Coronal Mass Ejections dur- ing Solar Cycle 24. International Journal of Astronomy and Astrophysics, 9, 191-199. https://doi.org/10.4236/ijaa.2019.93014 Received: May 9, 2019 Accepted: August 27, 2019 Published: August 30, 2019 Copyright © 2019 by author(s) and Scientific Research Publishing Inc. This work is licensed under the Creative Commons Attribution International License (CC BY 4.0). http://creativecommons.org/licenses/by/4.0/ Open Access