The polytropic behavior describes the relationship between macroscopic properties of
plasma species and provides useful information in understanding physical mechanisms in …

In late 1940 March, at least five significant solar flares were reported. They likely launched
interplanetary coronal mass ejections (ICMEs), and were associated with one of the largest …

Waves in plasma play an essential role in the energy transfer and plasma-heating
processes. This article discusses the in situ observation of Alfvén ion cyclotron (AIC) waves …

This paper reports, for the first time on a statistical basis, on the key role played by the
Alfvénic fluctuations in modulating the recovery phase of the geomagnetic storms, slowing …

A geomagnetic storm is a phenomenon of weakening of Earth's magnetic field from a few
hours to several days, which directly or indirectly affects navigation, transportation …

The sheath plasma of interplanetary coronal mass ejections (ICMEs) is highly compressed,
heated, turbulent, and magnetically intense relative to the ambient solar wind. In this Letter …

The Alfvén wave (AW) is the most common fluctuation present within the solar wind emitted
from the Sun. Whether or not AWs can originate after the collision of an Interplanetary …

Abstract Generally, Co-rotating Interaction Region (CIR) induced geomagnetic storms are
weak to moderate in magnitude. Moreover, CIRs can also drive intense storms when they …

The Forbush decrease (FD) and Geomagnetic storm (GS) are the two distinct space weather
events having common causing agents like interplanetary coronal mass ejection (ICME) or …

The excess speed of coronal mass ejection over the ambient solar wind in interplanetary
space generates a highly compressed, heated and turbulent shock-sheath. Here, for the first …