The magnetic field clock angle departure in the Venusian magnetosheath and its response to IMF rotation
We investigate the characteristics of interplanetary magnetic field (IMF) draping in the
Venusian magnetosheath using both Venus Express (VEX) observations and …
Venusian magnetosheath using both Venus Express (VEX) observations and …
Solar control of the pickup ion plume in the dayside magnetosheath of Venus
Abstract Using the 8.5‐year Venus Express measurements, we demonstrate the asymmetric
plasma distributions in the Venusian magnetosheath. An escaping plume is formed by …
plasma distributions in the Venusian magnetosheath. An escaping plume is formed by …
The dependence of the Venusian induced magnetosphere on the interplanetary magnetic field: An MHD study
The influences of the interplanetary magnetic field (IMF) on the induced magnetosphere of
Venus are investigated using a global multispecies magnetohydrodynamics (MHD) model …
Venus are investigated using a global multispecies magnetohydrodynamics (MHD) model …
[HTML][HTML] Magnetospheric Venus Space Explorers (MVSE) mission: A proposal for understanding the dynamics of induced magnetospheres
R Albers, H Andrews, G Boccacci, VDC Pires… - Acta Astronautica, 2024 - Elsevier
Induced magnetospheres form around planetary bodies with atmospheres through the
interaction of the solar wind with their ionosphere. Induced magnetospheres are highly …
interaction of the solar wind with their ionosphere. Induced magnetospheres are highly …
Properties of Mars' dayside low‐altitude induced magnetic field and comparisons with Venus
Mars and Venus have atmospheres but lack intrinsic dipole magnetic fields. Consequently,
the solar wind interaction at each planet results in the formation of an induced …
the solar wind interaction at each planet results in the formation of an induced …
A 3D Parametric Venusian Bow Shock Model with the Effects of Mach Number and Interplanetary Magnetic Field
Using global magnetohydrodynamics simulations, we have developed a three-dimensional
parametric model for the Venusian bow shock based on a generalized conic section function …
parametric model for the Venusian bow shock based on a generalized conic section function …
[HTML][HTML] Magnetospheric Physics in China: 2020–2021
CAO Jinbin, Y Junying - 空间科学学报, 2022 - cjss.ac.cn
In the past two years, many progresses were made in magnetospheric physics by the data of
OMNI, SuperMAG networks, Double Star Program, Cluster, THEMIS, RBSP, DMSP …
OMNI, SuperMAG networks, Double Star Program, Cluster, THEMIS, RBSP, DMSP …
Effects of the Parker spiral angle of the interplanetary magnetic field on the dawn-dusk asymmetry of the Martian magnetotail
G Li, H Lu, J Cao, Y Li, S Li - Astronomy & Astrophysics, 2023 - aanda.org
Context. The draping of the interplanetary magnetic field (IMF) around unmagnetized
planets induces a magnetotail with a two-lobe plasma structure. On Mars, due to the impact …
planets induces a magnetotail with a two-lobe plasma structure. On Mars, due to the impact …