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Force Analysis of Venus's Induced Magnetosphere: A Multifluid Hall–Magnetohydrodynamics Study
DOI: 10.3847/1538-4357/ada356 Bibcode: 2025ApJ...979..230C

Cao, Jinbin; Ge, Yasong; Lu, Haoyu +8 more

Understanding which processes control atmospheric escape and the loss of water from planetary environments is crucial. The ESA's Venus Express spacecraft has observed a significant depletion in Venus's upper atmosphere, driven by the solar wind. In such scenarios, the electromagnetic force can accelerate planetary ions to energies that allow them …

2025 The Astrophysical Journal
VenusExpress 0
Similarities and Differences between ICME-driven Shocks Observed by VEX (∼0.72 au) and WIND (∼1.0 au)
DOI: 10.3847/1538-4357/ada35b Bibcode: 2025ApJ...980....9R

Xu, Qi; Feng, Xueshang; Shen, Zhenning +7 more

The features of interplanetary shocks driven by interplanetary coronal mass ejections (ICMEs) observed by WIND (∼1.0 au) and Venus Express (VEX; ∼0.72 au) during the same period are statistically analyzed by comparing their similarities and differences. It is found that the proportion of ICME-driven shocks in all shocks decreases slightly from ∼0.…

2025 The Astrophysical Journal
VenusExpress 0
Influence of Solar Wind Variations on the Shapes of Venus' Plasma Boundaries Based on Venus Express Observations
DOI: 10.3847/1538-4357/ace7b1 Bibcode: 2023ApJ...954...95S

André, N.; Fedorov, A.; Futaana, Y. +10 more

The interaction between the solar wind and Venus creates an induced magnetosphere. The regions of the induced magnetosphere are separated by plasma boundaries, where their shapes and sizes are influenced by variations in the surrounding environment. Investigations of the boundaries and their variability can help us understand the solar wind's effe…

2023 The Astrophysical Journal
VenusExpress 7
Planar Magnetic Structures Downstream of Coronal Mass Ejection-driven Shocks in the Inner Heliosphere
DOI: 10.3847/1538-4357/acd245 Bibcode: 2023ApJ...951...47R

Xu, Qi; Feng, Xueshang; Shen, Zhenning +7 more

Planar magnetic structures (PMSs), characterized by interplanetary magnetic field vectors remaining parallel to a specific plane, are commonly observed in the solar wind, especially in the sheath region of interplanetary coronal mass ejections (ICMEs). In this study, PMS events in the 2 hr regions downstream of ICME-driven shocks were investigated…

2023 The Astrophysical Journal
SolarOrbiter VenusExpress 4
A New Tool for Understanding the Solar Wind-Venus Interaction: Three-dimensional Multifluid MHD Model
DOI: 10.3847/1538-4357/acba88 Bibcode: 2023ApJ...945...91D

Zhang, Tielong; Yao, Zhonghua; Dang, Tong +5 more

In this paper, we present a new tool to investigate the interaction of the solar wind with Venus with the approach of a global multifluid magnetohydrodynamics (MHD) model. The continuity, momentum, and energy equations for H+, O+, ${{\rm{O}}}_{2}^{+}$ , and ${\mathrm{CO}}_{2}^{+}$ are solved self-consistently together with Fa…

2023 The Astrophysical Journal
VenusExpress 3
Structure of a Quasi-parallel Shock Front
DOI: 10.3847/1538-4357/ad0b71 Bibcode: 2023ApJ...959..130B

Zhang, Tielong; Gedalin, Michael; Walker, Simon N. +2 more

The aim of this study is to compare observations of the magnetic field structure of observed quasi-parallel collisionless shock fronts with the results obtained analytically. A two-fluid analytic model of the shock front structure was derived under the assumptions that the shock is stationary and planar. The ion and electron kinetic pressures were…

2023 The Astrophysical Journal
VenusExpress 2
Influence of an Upstream Dynamic Pressure Pulse on Venus-Solar Wind Interaction by Multispecies Magnetohydrodynamic Simulation
DOI: 10.3847/1538-4357/acfca7 Bibcode: 2023ApJ...958..142L

Cao, Jinbin; Li, Yun; Xiong, Ruijing +4 more

As an unmagnetized planet, Venus does not have a global dipole magnetic field like Earth. The solar wind interacts directly with the Venusian ionosphere. In this paper, the interaction between solar wind and the Venusian upper atmosphere is investigated by conducting a three-dimensional multispecies magnetohydrodynamic (MHD) model, in which the Ve…

2023 The Astrophysical Journal
VenusExpress 2
Causes and Consequences of Magnetic Complexity Changes within Interplanetary Coronal Mass Ejections: A Statistical Study
DOI: 10.3847/1538-4357/ac3e60 Bibcode: 2022ApJ...927..102S

Lugaz, Noé; Scolini, Camilla; Winslow, Réka M. +3 more

We present the first statistical analysis of complexity changes affecting the magnetic structure of interplanetary coronal mass ejections (ICMEs), with the aim of answering the questions: How frequently do ICMEs undergo magnetic complexity changes during propagation? What are the causes of such changes? Do the in situ properties of ICMEs differ de…

2022 The Astrophysical Journal
VenusExpress 23
Multi-spacecraft Observations of the Evolution of Interplanetary Coronal Mass Ejections between 0.3 and 2.2 au: Conjunctions with the Juno Spacecraft
DOI: 10.3847/1538-4357/ac731a Bibcode: 2022ApJ...933..127D

Lugaz, Noé; Scolini, Camilla; Winslow, Réka M. +4 more

We present a catalog of 35 interplanetary coronal mass ejections (ICMEs) observed by the Juno spacecraft and at least one other spacecraft during its cruise phase to Jupiter. We identify events observed by MESSENGER, Venus Express, Wind, and STEREO with magnetic features that can be matched unambiguously with those observed by Juno. A multi-spacec…

2022 The Astrophysical Journal
Ulysses VenusExpress 19
Validation and Interpretation of a Three-dimensional Configuration of a Magnetic Cloud Flux Rope
DOI: 10.3847/1538-4357/ac7803 Bibcode: 2022ApJ...934...50H

Qiu, Jiong; Hu, Qiang; Jian, Lan K. +3 more

One strong magnetic cloud (MC) with a magnetic field magnitude reaching ~40 nT at 1 au during 2012 June 16-17 is examined in association with a preexisting magnetic flux rope (MFR) identified on the Sun. The MC is characterized by a quasi-three-dimensional (3D) flux rope model based on in situ measurements from the Wind spacecraft. The contents of…

2022 The Astrophysical Journal
SOHO VenusExpress 7