Imaging plasma density structures in the soft X-rays generated by solar wind charge exchange with neutrals
Both heliophysics and planetary physics seek to understand the complex nature of the solar
wind's interaction with solar system obstacles like Earth's magnetosphere, the ionospheres …
wind's interaction with solar system obstacles like Earth's magnetosphere, the ionospheres …
A review of Alfvénic turbulence in high‐speed solar wind streams: Hints from cometary plasma turbulence
Solar wind turbulence within high‐speed streams is reviewed from the point of view of
embedded single nonlinear Alfvén wave cycles, discontinuities, magnetic decreases (MDs) …
embedded single nonlinear Alfvén wave cycles, discontinuities, magnetic decreases (MDs) …
Automated Multi-Dataset Analysis (AMDA): An on-line database and analysis tool for heliospheric and planetary plasma data
V Génot, E Budnik, C Jacquey, M Bouchemit… - Planetary and Space …, 2021 - Elsevier
Accessing, visualizing and analyzing heterogeneous plasma datasets has always been a
tedious task that hindered students and senior researchers as well. Offering user friendly …
tedious task that hindered students and senior researchers as well. Offering user friendly …
A MAVEN case study of radial IMF at Mars: Impacts on the dayside ionosphere
The solar wind interaction with Mars controls the transfer of energy and momentum from the
solar wind into the magnetosphere, ionosphere and atmosphere, driving structure, and …
solar wind into the magnetosphere, ionosphere and atmosphere, driving structure, and …
Cold and warm electrons at comet 67P/Churyumov-Gerasimenko
AI Eriksson, IAD Engelhardt, M André… - Astronomy & …, 2017 - aanda.org
Context. Strong electron cooling on the neutral gas in cometary comae has been predicted
for a long time, but actual measurements of low electron temperature are scarce. Aims. Our …
for a long time, but actual measurements of low electron temperature are scarce. Aims. Our …
The birth and growth of a solar wind cavity around a comet – Rosetta observations
The Rosetta mission provided detailed observations of the growth of a cavity in the solar
wind around comet 67P/Churyumov–Gerasimenko. As the comet approached the Sun, the …
wind around comet 67P/Churyumov–Gerasimenko. As the comet approached the Sun, the …
Evolution of the ion environment of comet 67P during the Rosetta mission as seen by RPC-ICA
Rosetta has followed comet 67P from low activity at more than 3.6 au heliocentric distance to
high activity at perihelion (1.24 au) and then out again. We provide a general overview of the …
high activity at perihelion (1.24 au) and then out again. We provide a general overview of the …
Impact of radial interplanetary magnetic fields on the inner coma of comet 67P/Churyumov-Gerasimenko-Hybrid simulations of the plasma environment
Context. The direction of the interplanetary magnetic field determines the nature of the
interaction between a Solar System object and the solar wind. For comets, it affects the …
interaction between a Solar System object and the solar wind. For comets, it affects the …
Diamagnetic region (s): structure of the unmagnetized plasma around Comet 67P/CG
The ESA's comet chaser Rosetta has monitored the evolution of the ionized atmosphere of
comet 67P/Churyumov–Gerasimenko (67P/CG) and its interaction with the solar wind …
comet 67P/Churyumov–Gerasimenko (67P/CG) and its interaction with the solar wind …
Ion velocity and electron temperature inside and around the diamagnetic cavity of comet 67P
E Odelstad, AI Eriksson, FL Johansson… - Journal of …, 2018 - Wiley Online Library
A major point of interest in cometary plasma physics has been the diamagnetic cavity, an
unmagnetized region in the innermost part of the coma. Here we combine Langmuir and …
unmagnetized region in the innermost part of the coma. Here we combine Langmuir and …