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 …

In this paper, we present a detailed study of the effects of the interplanetary magnetic field
(IMF) strength on the foreshock properties at small and large scales. Two simulation runs …

Studies of Mercury's foreshock have analyzed in detail the properties of ultra-low frequency
waves. However, an open question remains in regards to understanding favorable …

This review examines ultra-low frequency (ULF) waves across different planetary
environments, focusing on Earth, Mercury, and Saturn. Data from spacecraft missions …

Using direct numerical simulations (DNSs), the interaction between linear waves and
turbulence under the compressible magnetohydrodynamic (CMHD) approach was studied …

We perform the first statistical analysis of the main properties of waves observed in the 0.05–
0.41 Hz frequency range in the Hermean foreshock by the MErcury Surface, Space …

We present a statistical analysis on the variability of the incompressible energy cascade rate
in the solar wind around Mars, making use of an exact relation for fully developed turbulence …

The foreshock is a region of space upstream of the Earth's bow shock extending along the
interplanetary magnetic field (IMF). It is permeated by shock-reflected ions and electrons …

The location and spatial extent of the region populated by the foreshock waves depend on
the IMF orientation. We performed a systematic statistical study of wave activity in the …

The statistical properties of ULF waves observed upstream of Venus foreshock are
investigated. The study is restricted to waves which are observed well below the local proton …