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Magnetospheric Venus Space Explorers (MVSE) mission: A proposal for understanding the dynamics of induced magnetospheres.

Authors :
Albers, Roland
Andrews, Henrik
Boccacci, Gabriele
Pires, Vasco D.C.
Laddha, Sunny
Lundén, Ville
Maraqten, Nadim
Matias, João
Krämer, Eva
Schulz, Leonard
Palanca, Ines Terraza
Teubenbacher, Daniel
Baskevitch, Claire
Covella, Francesca
Cressa, Luca
Moreno, Juan Garrido
Gillmayr, Jana
Hollowood, Joshua
Huber, Kilian
Kutnohorsky, Viktoria
Source :
Acta Astronautica. Aug2024, Vol. 221, p194-205. 12p.
Publication Year :
2024

Abstract

Induced magnetospheres form around planetary bodies with atmospheres through the interaction of the solar wind with their ionosphere. Induced magnetospheres are highly dependent on the solar wind conditions and have only been studied with single spacecraft missions in the past. Without simultaneous measurements of solar wind variations and phenomena in the magnetosphere, establishing a link between both can only be done indirectly, using statistics over a large set of measurements. This gap in knowledge could be addressed by a multi-spacecraft plasma mission, optimized for studying global spatial and temporal variations in the magnetospheric system around Venus, which hosts the most prominent example of an induced magnetosphere in our solar system. The MVSE mission comprises four satellites, of which three are identical scientific spacecraft, carrying the same suite of instruments probing different regions of the induced magnetosphere and the solar wind simultaneously. The fourth spacecraft is the transfer vehicle which acts as a relay satellite for communications at Venus. In this way, changes in the solar wind conditions and extreme solar events can be observed, and their effects can be quantified as they propagate through the Venusian induced magnetosphere. Additionally, energy transfer in the Venusian induced magnetosphere can be investigated. The scientific payload includes instrumentation to measure the magnetic field, electric field, and ion–electron velocity distributions. This study presents the scientific motivation for the mission as well as requirements and the resulting mission design. Concretely, a mission timeline along with a complete spacecraft design, including mass, power, communication, propulsion and thermal budgets are given. This mission was initially conceived at the Alpbach Summer School 2022 and refined during a week-long study at ESA's Concurrent Design Facility in Redu, Belgium. • Multi-spacecraft plasma physics mission concept to Venus. • Dynamics of induced magnetospheres due to variations in the solar wind. • Magnetospheric reaction due to extreme solar events. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00945765
Volume :
221
Database :
Academic Search Index
Journal :
Acta Astronautica
Publication Type :
Academic Journal
Accession number :
177873345
Full Text :
https://doi.org/10.1016/j.actaastro.2024.05.017