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View article: Detectability of Dust and Ion Tails of Interstellar Comet 3I/ATLAS by Europa Clipper
Detectability of Dust and Ion Tails of Interstellar Comet 3I/ATLAS by Europa Clipper Open
The Europa Clipper spacecraft is located about 1 au downstream from the interstellar comet 3I/ATLAS around its perihelion. Here we model the propagation of pickup ions and cometary dust originating from 3I/ATLAS to examine their detectabil…
View article: Observational Characteristics of Electron Distributions in the Martian Induced Magnetotail
Observational Characteristics of Electron Distributions in the Martian Induced Magnetotail Open
Mars's magnetotail represents a unique case within the solar system, embodying both intrinsic and induced magnetic fields. Yet, the electron dynamics within this region have remained largely unexplored. Utilizing nine years of electron and…
View article: Charging effects on <i>Rosetta</i> dust measurements
Charging effects on <i>Rosetta</i> dust measurements Open
Dust particles released from comet 67P/Churyumov-Gerasimenko collect electrostatic charges. Their motion is influenced by the electric fields induced by the flow of the solar wind and by the charging of the Rosetta spacecraft itself. Dust …
View article: Electrostatic Dust Analyzer for Dust Transport Measurements on the Lunar Surface
Electrostatic Dust Analyzer for Dust Transport Measurements on the Lunar Surface Open
Lunar dust charging and transport is a more than five-decade-old problem. A high-fidelity and flight-qualified Electrostatic Dust Analyzer (EDA) has been developed to measure the charge, velocity, mass (size), and flux of electrostatically…
View article: The Comet Interceptor Mission
The Comet Interceptor Mission Open
View article: The Value of the Moon for Heliophysics
The Value of the Moon for Heliophysics Open
International audience
View article: Solar-wind electron precipitation on weakly magnetized bodies: The planet Mercury
Solar-wind electron precipitation on weakly magnetized bodies: The planet Mercury Open
Rocky objects in the Solar System (such as planets, asteroids, moons, and comets) undergo a complex interaction with the flow of magnetized, supersonic plasma emitted from the Sun called solar wind. We address the interaction of such a flo…
View article: Fully-kinetic global simulations of Mercury's magnetosphere in support to BepiColombo
Fully-kinetic global simulations of Mercury's magnetosphere in support to BepiColombo Open
Mercury is the only telluric planet of the solar system, apart from Earth, possessing an intrinsic magnetic field.This magnetic field shapes (and it is shaped by) the plasma dynamics around the planet, defining the Herman magnetosphere, an…
View article: Solar wind interaction with a comet: evolution, variability, and implication
Solar wind interaction with a comet: evolution, variability, and implication Open
Once a cometary plasma cloud has been created through ionisation of the cometary neutrals, it presents an obstacle to the solar wind and the magnetic field within it. The acceleration and incorporation of the cometary plasma by the solar w…
View article: Cold electrons at a weakly outgassing comet&#160;
Cold electrons at a weakly outgassing comet  Open
<p>The Rosetta spacecraft rendezvoused with comet 67P/Churyumov-Gerasimenko in August 2014 and escorted it for two years until September 2016. The plasma surrounding the comet was probed by the Rosetta Plasma Consortium (RPC), compri…
View article: Electron dynamics in Mercury&#8217;s magnetosphere using a global fully-kinetic model
Electron dynamics in Mercury’s magnetosphere using a global fully-kinetic model Open
<p align="justify"><span lang="en-US">Mercury is the only telluric planet of the solar system, other than Earth, with an intrinsic magnetic field. Thus, the Hermean surface is shielded from the impinging sol…
View article: The source of electrons at a weakly outgassing comet
The source of electrons at a weakly outgassing comet Open
<p>The Rosetta spacecraft escorted comet 67P/Churyumov-Gerasimenko for two years along its orbit, from Aug 2014 to Sep 2016, observing the evolution of the comet from a close perspective. The Rosetta Plasma Consortium (RPC) monitored…
View article: Solar-wind electron precipitation on weakly magnetized bodies: the\n planet Mercury
Solar-wind electron precipitation on weakly magnetized bodies: the\n planet Mercury Open
Mercury is the archetype of a weakly magnetized, airless, telluric body\nimmersed in the solar wind. Due to the lack of any substantial atmosphere, the\nsolar wind directly precipitates on Mercury's surface. Using a 3D fully-kinetic\nself-…
View article: Electron dynamics in small magnetospheres
Electron dynamics in small magnetospheres Open
Context. The planet Mercury possesses a small but highly dynamic magnetosphere in which the role and dynamics of electrons are still largely unknown. Aims. We aim to model the global dynamics of solar-wind electrons impinging on Mercury’s …
View article: Electron dynamics in small magnetospheres: insights from global fully-kinetic plasma simulations of planet Mercury
Electron dynamics in small magnetospheres: insights from global fully-kinetic plasma simulations of planet Mercury Open
The planet Mercury possesses a small but highly dynamic magnetosphere in which the role and dynamics of electrons are still largely unknown. We aim at modeling the global dynamics of solar wind electrons impinging on Mercury's magnetospher…
View article: Three-dimensional Particle-in-Cell (PIC) simulations of non-dipolar minimagnetospheres and comparison to the experiment.
Three-dimensional Particle-in-Cell (PIC) simulations of non-dipolar minimagnetospheres and comparison to the experiment. Open
<p>Magnetospheres are formed when plasma flow interacts with an external source of the magnetic field. Objects (with a size comparable to or less than the ion inertial length or ion gyroradius) formed by relatively weak magnetic fiel…
View article: A Fully Kinetic Perspective on Weakly Active Comets: Symmetric versus Asymmetric Outgassing
A Fully Kinetic Perspective on Weakly Active Comets: Symmetric versus Asymmetric Outgassing Open
<p>For more than two years, ESA’s Rosetta mission measured the complex and ever-evolving plasma environment surrounding comet 67P/Churyumov-Gerasimenko. In this work, we explore the structure and dynamics of the near-comet …
View article: Full-kinetic global simulations of the plasma environment at Mercury: a model from planetary to electrons scales to support BepiColombo
Full-kinetic global simulations of the plasma environment at Mercury: a model from planetary to electrons scales to support BepiColombo Open
<p>Mercury is the only telluric planet of the solar system, other than Earth, with an intrinsic magnetic field. Thus, the Hermean surface is shielded from the impinging solar wind via the presence of an “Earth-like̶…
View article: A collisional test-particle model of electrons at a comet
A collisional test-particle model of electrons at a comet Open
We have developed the first 3D collisional model of electrons at a comet, which we use to examine the impact of electron-neutral collisions in the weakly outgassing regime. The test-particle Monte Carlo model uses electric and magnetic fie…
View article: Laboratory Simulation of Solar Wind Interaction With Lunar Magnetic Anomalies
Laboratory Simulation of Solar Wind Interaction With Lunar Magnetic Anomalies Open
Magnetic anomalies on the surface of the Moon interact with the solar wind plasma flow, resulting in both magnetic and electrostatic deflection/reflection of charged particles. Consequently, surface charging in these regions differs from r…
View article: The Plasma Environment Surrounding the Reiner Gamma Magnetic Anomaly
The Plasma Environment Surrounding the Reiner Gamma Magnetic Anomaly Open
Reiner Gamma is a prime target for low‐orbiting spacecraft or even surface‐landed missions in the near future. The region hosts a prominent lunar swirl that is co‐located with a strong and well‐structured magnetic anomaly. We simulate and …
View article: Dynamics of electrostatically lofted dust on airless planetary bodies
Dynamics of electrostatically lofted dust on airless planetary bodies Open
View article: Author Correction: Far-ultraviolet aurora identified at comet 67P/Churyumov-Gerasimenko
Author Correction: Far-ultraviolet aurora identified at comet 67P/Churyumov-Gerasimenko Open
View article: The Plethora of Science Afforded by a Lunar Swirl
The Plethora of Science Afforded by a Lunar Swirl Open
Whitepaper #166 submitted to the Planetary Science and Astrobiology Decadal Survey 2023-2032. Topics: surface/geological evolution; Mercury and/or the Moon; other science themes: Physics, Heliophysics, Magnetohydrodynamics, Volcanology, IS…
View article: NanoSWARM: NanoSatellites for Space Weathering, Surface Water, Solar Wind, and Remanent Magnetism
NanoSWARM: NanoSatellites for Space Weathering, Surface Water, Solar Wind, and Remanent Magnetism Open
The NanoSWARM mission concept is a detailed investigation of particles and magnetic fields to help characterize the surfaces of airless planetary bodies, their volatile element distributions, and their geophysical histories.NanoSWARM inves…
View article: Numerical and laboratory studies of magnetic enhancements produced by solar wind interaction with Lunar crustal magnetic fields
Numerical and laboratory studies of magnetic enhancements produced by solar wind interaction with Lunar crustal magnetic fields Open
<p>In this study, we use a combination of 3D Particle-in-Cell (PIC) simulations and a laboratory experiment to investigate the dynamics of solar wind - Moon interaction. It is known that the Moon has no global magnetic field, but the…
View article: On ion temperature dependence of symmetric magnetic reconnection
On ion temperature dependence of symmetric magnetic reconnection Open
<p>Various simulations of collisionless magnetic reconnection reveal that the process is typically fast, with the reconnection rate being of the order of 0.1. Systematic numerical and observational studies of upstream parameters depe…
View article: Electron cooling at a weakly outgassing comet
Electron cooling at a weakly outgassing comet Open
<p>The Rosetta spacecraft arrived at comet 67P in August 2014 and then escorted it for 2 years along its orbit. Throughout this escort phase, two plasma instruments (Mutual Impedance Probe, MIP; and Langmuir Probe, LAP) measured a po…
View article: Cold ion energization at separatrices during magnetic reconnection
Cold ion energization at separatrices during magnetic reconnection Open
Separatrices of magnetic reconnection host intense perpendicular Hall electric fields. The fields are produced by the decoupling of the ion and electron components and are associated with the in-plane electrostatic potential drop between t…
View article: Cross-comparison of global simulation models applied to Mercury’s dayside magnetosphere
Cross-comparison of global simulation models applied to Mercury’s dayside magnetosphere Open