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 …

Dayside transients, such as hot flow anomalies, foreshock bubbles, magnetosheath jets, flux
transfer events, and surface waves, are frequently observed upstream from the bow shock …

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

This chapter focuses on the range of low frequency electromagnetic modes observed at and
upstream of collisionless shocks in the heliosphere. It discusses a specific class of whistler …

The Earth's bow shock is the most studied example of a collisionless shock in the solar
system. It is also widely used to model or predict the behaviour at other astrophysical shock …

The physics of collisionless shocks is a very broad topic which has been studied for more
than five decades. However, there are a number of important issues which remain …

This unique, authoritative book introduces and accurately depicts the current state-of-the art
in the field of space storms. Professor Koskinen, renowned expert in the field, takes the basic …

The solar wind interaction with Mars controls the transfer of energy and momentum from the
solar wind into the magnetosphere, ionosphere and atmosphere, driving structure, and …

When the interplanetary magnetic field is oriented such that the angle between the upstream
magnetic field and the nominal bow shock normal is small (θBn< 45◦), a much more complex …

Context. We study the solar energetic particle (SEP) event observed on 9 October 2021 by
multiple spacecraft, including Solar Orbiter. The event was associated with an M1. 6 flare, a …