Shock waves are an important feature of solar system plasmas, from the solar corona out to
the edge of the heliosphere. This engaging introduction to collisionless shocks in space …

Shock waves are associated with multiple powerful coherent radio emissions within the
heliosphere and local interstellar medium. The radio emissions definitely driven by shocks …

Type II radio bursts drift in frequency as shock waves and coronal mass ejections (CMEs)
move through the Sun's corona and the solar wind. This paper extends the theoretical …

A new method for remote sensing of the quasiperpendicular part of the bow shock surface is
presented. The method is based on analysis of high frequency electric field fluctuations …

A one‐dimensional full particle‐in‐cell (PIC) code is utilized to investigate energetic electron
bursts produced at a nonstationary quasi‐perpendicular shock. A number of electrons are …

In this paper, the second in a two paper series, we quantitatively compare a detailed theory
for type II solar radio bursts with observations and extract the parameters of the associated …

Test particle calculations are performed to investigate the effects of different shock
parameters on electron distributions upstream and downstream of quasi‐perpendicular …

Recent simulation results have revealed that energetic electron bursts are produced
cyclically at the shock reformation period upstream of reforming shocks and are qualitatively …

Shock drift acceleration is one of the important mechanisms for electron acceleration
associated with magnetic mirror reflection along the magnetic field in a quasi-perpendicular …

The doctoral thesis is devoted to the investigation of wave processes in the vicinity of space
plasma shocks. The numerical modelling of the Langmuir wave propagation in plasma with …