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The Analysis of Interplanetary Shocks Associated with Six Major Geo Effective Coronal Mass Ejections during Solar Cycle 24

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Figure

Table 1. Details for major geo-effective CMEs with associated flare. Last column shows the detail of generated interplanetary shock with DST value
Table 2. Difference between actual transit time with various acceleration cessation dis-tances (0.7 AU, 0.6 AU and 0.5 AU) for Equations (3)-(5)
Figure 1. Comparison between actual transit time (TT) of IP shock and estimated transit time for various acceleration cessation distances (0.7 AU, 0.6 AU and 0.5 AU) obtained from different acceleration-speed Equations (3)-(5) in plot (a), (b) and (c) resp
Figure 2. Transit time calculated using second-order speed (a) at final distance (b) at 20 solar radii
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