Transmission of foreshock waves through Earth's bow shock
The Earth's magnetosphere and its bow shock, which is formed by the interaction of the
supersonic solar wind with the terrestrial magnetic field, constitute a rich natural laboratory …
supersonic solar wind with the terrestrial magnetic field, constitute a rich natural laboratory …
Connection between foreshock structures and the generation of magnetosheath jets: Vlasiator results
Earth's magnetosheath consists of shocked solar wind plasma that has been compressed
and slowed down at the Earth's bow shock. Magnetosheath jets are pulses of enhanced …
and slowed down at the Earth's bow shock. Magnetosheath jets are pulses of enhanced …
Quasi‐Parallel Shock Reformation Seen by Magnetospheric Multiscale and Ion‐Kinetic Simulations
Shock waves in collisionless plasmas are among the most efficient particle accelerators in
space. Shock reformation is a process important to plasma heating and acceleration, but …
space. Shock reformation is a process important to plasma heating and acceleration, but …
Magnetosheath jet evolution as a function of lifetime: Global hybrid-Vlasov simulations compared to MMS observations
Magnetosheath jets are regions of high dynamic pressure, which can traverse from the bow
shock towards the magnetopause. Recent modelling efforts, limited to a single jet and a …
shock towards the magnetopause. Recent modelling efforts, limited to a single jet and a …
Probing the foreshock wave boundary with single spacecraft techniques
In space physics, wave measurements typically use a small number of datapoints due to
limited available spacecraft. Common single‐spacecraft wave vector analysis techniques …
limited available spacecraft. Common single‐spacecraft wave vector analysis techniques …
A global view of Pc3 wave activity in near-Earth space: Results from hybrid-Vlasov simulations
Ultra-low frequency (ULF) waves in the Pc3 range, with periods between 10–45 s, are
routinely observed in Earth's dayside magnetosphere. They are thought to originate in the …
routinely observed in Earth's dayside magnetosphere. They are thought to originate in the …
Helium in the Earth's foreshock: a global Vlasiator survey
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 …
interplanetary magnetic field (IMF). It is permeated by shock-reflected ions and electrons …
Hybrid-Vlasov simulation of soft X-ray emissions at the Earth's dayside magnetospheric boundaries
Solar wind charge exchange produces emissions in the soft X-ray energy range which can
enable the study of near-Earth space regions such as the magnetopause, the …
enable the study of near-Earth space regions such as the magnetopause, the …
Asymmetries in the Earth's dayside magnetosheath: results from global hybrid-Vlasov simulations
L Turc, V Tarvus, AP Dimmock… - Annales …, 2020 - angeo.copernicus.org
Bounded by the bow shock and the magnetopause, the magnetosheath forms the interface
between solar wind and magnetospheric plasmas and regulates solar wind–magnetosphere …
between solar wind and magnetospheric plasmas and regulates solar wind–magnetosphere …
[HTML][HTML] Foreshock cavitons and spontaneous hot flow anomalies: a statistical study with a global hybrid-Vlasov simulation
The foreshock located upstream of Earth's bow shock hosts a wide variety of phenomena
related to the reflection of solar wind particles from the bow shock and the subsequent …
related to the reflection of solar wind particles from the bow shock and the subsequent …