Search Publications

LatHyS global hybrid simulation of the BepiColombo second Venus flyby
DOI: 10.1016/j.pss.2022.105499 Bibcode: 2022P&SS..21805499A

André, N.; Fedorov, A.; Sauvaud, J. -A. +23 more

Plasma and magnetic field observations by BepiColombo during its 2nd Venus flyby in August 10, 2021 have been examined and compared with the newly developed global hybrid simulation LatHyS for the Venusian environment. The LatHyS-Venus simulation was first validated by a comparison with Venus Express observations obtained during average solar wind…

2022 Planetary and Space Science
BepiColombo SolarOrbiter VenusExpress 4
Calibration of ISA accelerometer sensing axes for the BepiColombo mission
DOI: 10.1016/j.pss.2021.105396 Bibcode: 2022P&SS..21105396L

Lucente, Marco; Lefevre, Carlo; Fiorenza, Emiliano +3 more

ISA is a three-axis accelerometer embarked on-board BepiColombo, a joint ESA/JAXA space mission launched on the 19th of October 2018 at 22.45 (local time) and devoted to put two spacecraft (MPO and MMO) around Mercury (2025), for a deeper investigation of the planet and its environment. ISA aims at measuring, directly and not by modelli…

2022 Planetary and Space Science
BepiColombo 1
Localization of cosmic gamma-ray bursts in interplanetary space with MGNS/BepiColombo and HEND/Mars Odyssey experiments
DOI: 10.1016/j.pss.2022.105594 Bibcode: 2022P&SS..22405594K

Golovin, D. V.; Kozyrev, A. S.; Litvak, M. L. +3 more

This paper describes the methods and results for the localization by triangulation of cosmic gamma-ray bursts (GRBs) independently observed by two space experiments: the Mercury Gamma-ray and Neutron Spectrometer (MGNS) and the High Energy Neutron Detector (HEND). MGNS is onboard the MPO/BepiColombo mission and on a stage of cruise to Mercury wher…

2022 Planetary and Space Science
BepiColombo 0
Cross-comparison of global simulation models applied to Mercury's dayside magnetosphere
DOI: 10.1016/j.pss.2021.105176 Bibcode: 2021P&SS..19805176A

André, N.; Budnik, E.; Génot, V. +14 more

We present the first comparison of multiple global simulations of the solar wind interaction with Mercury's dayside magnetosphere, conducted in the framework of the international collaborative project SHOTS - Studies on Hermean magnetosphere Oriented Theories and Simulations. Two 3D magnetohydrodynamic and two 3D hybrid simulation codes are used t…

2021 Planetary and Space Science
BepiColombo 15
Orbital evolution of the BepiColombo Mercury Planetary Orbiter (MPO) in the gravity field of Mercury
DOI: 10.1016/j.pss.2021.105195 Bibcode: 2021P&SS..20005195H

Oberst, Jürgen; Hussmann, Hauke; Stark, Alexander +2 more

We assessed the impact of the uncertainties in the gravity field harmonic coefficients of Mercury on the orbital evolution of the Mercury Planetary Orbiter (MPO), part of the European-Japanese BepiColombo mission. We used in our simulations the most recent estimation of the gravity field model of Mercury determined from radio tracking data of the …

2021 Planetary and Space Science
BepiColombo 3
Comprehensive in-orbit performance evaluation of the BepiColombo Laser Altimeter (BELA)
DOI: 10.1016/j.pss.2020.105088 Bibcode: 2021P&SS..19505088H

Thomas, Nicolas; Hussmann, Hauke; Pommerol, Antoine +7 more

The BepiColombo Laser Altimeter (BELA) is on its way to Mercury on board the Mercury Planetary Orbiter (MPO), one of the two spacecraft of the BepiColombo mission. It will arrive at Mercury in December 2025 and start measurements of Mercury's surface and environment. The goal of this study is to analyze the performance of BELA by using a comprehen…

2021 Planetary and Space Science
BepiColombo 2
The performance of the BepiColombo Laser Altimeter (BELA) prior launch and prospects for Mercury orbit operations
DOI: 10.1016/j.pss.2018.04.017 Bibcode: 2018P&SS..159...84S

Oberst, J.; Stark, A.; Steinbrügge, G. +2 more

We explore the perspectives of the BepiColombo Laser Altimeter (BELA) onboard ESA / JAXA's Mercury mission BepiColombo and present an updated semi-analytical instrument performance model, in which we estimate signal-to-noise ratio, single shot probability of false detection, range errors and the accuracy of pulse width reconstruction. The model is…

2018 Planetary and Space Science
BepiColombo 21