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Future opportunities in solar system plasma science through ESA's exploration programme
Umeå University, Faculty of Science and Technology, Department of Physics. Swedish Institute of Space Physics, Kiruna, Sweden.ORCID iD: 0000-0001-5494-5374
School of Physics and Astronomy, University of Leicester, University Road, Leicester, United Kingdom.
School of Physics and Astronomy, University of Leicester, University Road, Leicester, United Kingdom.
2024 (English)In: npj Microgravity, E-ISSN 2373-8065, Vol. 10, no 1, article id 29Article, review/survey (Refereed) Published
Abstract [en]

The solar wind interacts with all solar system bodies, inducing different types of dynamics depending on their atmospheric and magnetic environments. We here outline some key open scientific questions related to this interaction, with a focus on the Moon and Mars, that may be addressed by future Mars and Moon missions by the European Space Agency's Human and Robotic Exploration programme. We describe possible studies of plasma interactions with bodies with and without an atmosphere, using multi-point and remote measurements, and energetic particle observations, as well as recommend some actions to take.

Place, publisher, year, edition, pages
Springer Nature, 2024. Vol. 10, no 1, article id 29
National Category
Fusion, Plasma and Space Physics Astronomy, Astrophysics and Cosmology
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URN: urn:nbn:se:umu:diva-223247DOI: 10.1038/s41526-024-00373-9ISI: 001185286500001PubMedID: 38486087Scopus ID: 2-s2.0-85188029974OAI: oai:DiVA.org:umu-223247DiVA, id: diva2:1852609
Available from: 2024-04-18 Created: 2024-04-18 Last updated: 2024-04-18Bibliographically approved

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fulltext(537 kB)43 downloads
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Holmström, Mats

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CiteExportLink to record
Permanent link

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Citation style
  • apa
  • ieee
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  • en-GB
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