This paper focuses on the interactions between the fast solar wind from coronal holes and
the intervening slower solar wind, leading to the creation of stream interaction regions that …

Alfvénic component of MHD turbulence damps Alfvénic waves. The consequences of this
effect are important for many processes, from cosmic ray (CR) propagation to launching …

This paper considers turbulent damping of Alfvén waves in magnetized plasmas. We identify
two cases of damping, one related to damping of cosmic-ray streaming instability, the other …

Context. Interplanetary coronal mass ejections (ICMEs) are the interplanetary manifestations
of solar eruptions. The overtaken solar wind forms a sheath of compressed plasma at the …

We present an analytical diffusion–expansion Forbush decrease (FD) model ForbMod,
which is based on the widely used approach of an initially empty, closed magnetic structure …

The intensity of galactic cosmic rays (GCRs) is modulated by solar activity on various
timescales. In this study, we performed comprehensive numerical modeling of the solar …

In this paper, Forbush decrease (FD) profiles are compared for events associated with (i)
coronal mass ejections from active regions accompanied by solar flares (AR CMEs),(ii) …

Interplanetary coronal mass ejections (ICMEs) are the counterparts of coronal mass
ejections (CMEs) that extend in the interplanetary (IP) space and interact with the underlying …

Galactic cosmic-ray (GCR) energy spectra observed in the inner heliosphere are modulated
by the solar activity, the solar polarity and structures of solar and interplanetary origin. A high …

Interplanetary coronal mass ejections (ICMEs) are known to modify the structure of the solar
wind as well as interact with the space environment of planetary systems. Their large …