Abstract:
Various remote and in situ observations, along with several models, simulations, and kinetic studies, have been
proposed in recent years, suggesting that the morphology of an interplanetary coronal mass ejection (ICME)
magnetic cloud can vary from cylindrical, elliptical, toroidal, flattened, pancaked, etc. Recently, Raghav et al.
proposed for the first time a unique morphological characteristic of an ICME magnetic cloud at 1 au that showed
characteristics of a planar magnetic structure, using in situ data from the ACE spacecraft. In this study, we
statistically investigate the plasma properties of planar and nonplanar ICMEs from 1998–2017 at 1 au. The detailed
study of 469 ICMEs suggests that 136 (∼29%) ICMEs are planar, whereas 333 (∼71%) are nonplanar.
Furthermore, total interplanetary magnetic field strength, average plasma parameters, i.e., plasma density, beta,
thermal pressure, and magnetic pressure in planar ICME, are significantly higher than in the nonplanar ICME.
Also, we noticed that the thickness of planar ICMEs is less compared to nonplanar ICMEs. This analysis
demonstrates that planar ICMEs are formed due to the high compression of ICME. Moreover, we also observed the
southward/northward magnetic field component’s double strength during planar ICMEs compared to nonplanar
ICMEs. It implies that planar ICMEs are more geoeffective than nonplanar ICMEs.
