Plasma wave investigation (PWI) aboard BepiColombo Mio on the trip to the first measurement of electric fields, electromagnetic waves, and radio waves around …

Y Kasaba, H Kojima, M Moncuquet, JE Wahlund… - Space Science …, 2020 - Springer
Abstract The Plasma Wave Investigation (PWI) aboard the BepiColombo Mio (Mercury
Magnetospheric Orbiter, MMO) will enable the first observations of electric fields, plasma …

The plasma environment of comet 67P/Churyumov-Gerasimenko

C Goetz, E Behar, A Beth, D Bodewits, S Bromley… - Space Science …, 2022 - Springer
The environment of a comet is a fascinating and unique laboratory to study plasma
processes and the formation of structures such as shocks and discontinuities from electron …

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 …

Plasma source and loss at comet 67P during the Rosetta mission

KL Heritier, M Galand, P Henri, FL Johansson… - Astronomy & …, 2018 - aanda.org
Context. The Rosetta spacecraft provided us with a unique opportunity to study comet
67P/Churyumov–Gerasimenko (67P) from a close perspective and over a 2-yr time period …

The influence of spacecraft charging on low‐energy ion measurements made by RPC‐ICA on Rosetta

S Bergman, G Stenberg Wieser… - Journal of …, 2020 - Wiley Online Library
Spacecraft charging is problematic for low‐energy plasma measurements. The charged
particles are attracted to or repelled from the charged spacecraft, affecting both the energy …

A charging model for the Rosetta spacecraft

FL Johansson, AI Eriksson, N Gilet, P Henri… - Astronomy & …, 2020 - aanda.org
Context. The electrostatic potential of a spacecraft, VS, is important for the capabilities of in
situ plasma measurements. Rosetta has been found to be negatively charged during most of …

Ion composition at comet 67P near perihelion: Rosetta observations and model-based interpretation

KL Heritier, K Altwegg, H Balsiger… - Monthly Notices of …, 2017 - academic.oup.com
We present the ion composition in the coma of comet 67P with newly detected ion species
over the 28–37 u mass range, probed by Rosetta Orbiter Spectrometer for Ion and Neutral …

Measurements of the electrostatic potential of Rosetta at comet 67P

E Odelstad, G Stenberg-Wieser… - Monthly Notices of …, 2017 - academic.oup.com
We present and compare measurements of the spacecraft potential (V s/c) of the Rosetta
spacecraft throughout its stay in the inner coma of comet 67P/Churyumov–Gerasimenko, by …

Observations of a mix of cold and warm electrons by RPC-MIP at 67P/Churyumov-Gerasimenko

N Gilet, P Henri, G Wattieaux, N Traoré… - Astronomy & …, 2020 - aanda.org
Context. The Mutual Impedance Probe (MIP) of the Rosetta Plasma Consortium (RPC)
onboard the Rosetta orbiter which was in operation for more than two years, between …

The influence of varying spacecraft potentials and Debye lengths on in situ low‐energy ion measurements

S Bergman, G Stenberg Wieser… - Journal of …, 2020 - Wiley Online Library
Low‐energy ions are difficult to measure, mainly due to spacecraft charging. The ions are
attracted to or repelled from the charged surface prior to detection, which changes both the …