Interplanetary coronal mass ejections (ICMEs) are large-scale heliospheric transients that
originate from the Sun. When an ICME is sufficiently faster than the preceding solar wind, a …

Abstract Interplanetary Coronal Mass Ejections (ICMEs), their possible shocks and sheaths,
and co-rotating interaction regions (CIRs) are the primary large-scale heliospheric structures …

The 1–2 September 1859 magnetic storm was the most intense in recorded history on the
basis of previously reported ground observations and on newly reduced ground‐based …

In particular during the descending phase of the solar cycle, Alfvén waves in the high-speed
solar wind streams are a major form of interplanetary disturbances. The fluctuating …

This two-part book is devoted to classic fundamentals and current practices and
perspectives of modern plasma astrophysics. This second part discusses the physics of …

We investigate the spectral properties of the electromagnetic fluctuations of sub-ion scale
turbulence in weakly collisional, low-beta plasmas using a two-field isothermal gyrofluid …

The turbulent flows and tangled magnetic fields of the Earth's plasma sheet are explored
theoretically and by means of ISEE‐2 plasma and magnetic‐field measurements. The goal …

Kelvin–Helmholtz instability plays a particularly important role in plasma transport at
magnetospheric boundaries because it can control the development of a turbulent boundary …

Magnetic turbulence is found in most space plasmas, including the Earth's magnetosphere,
and the interaction region between the magnetosphere and the solar wind. Recent …

We investigate the relative role of various types of solar wind streams in generation of
magnetic storms. On the basis of the OMNI data of interplanetary measurements for the …