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X-ray studies of solar system objects: Past, present, and the next decade

Branduardi-Raymont, G; (2017) X-ray studies of solar system objects: Past, present, and the next decade. Astronomische Nachrichten , 338 (2-3) pp. 188-194. 10.1002/asna.201713329. Green open access

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Abstract

This paper presents an overview of the remarkable progress that X-ray studies of solar system objects have delivered over the past three decades, covering research that encompasses remote observations with XMM-Newton and Chandra, in situ measurements by planetary missions, and models of solar wind propagation from 1 AU. The future of X-ray exploration of the solar system in the next decade is bright, counting on the continuing excellent imaging and spectral performance of XMM-Newton instruments, which is most effective when combined with the outstanding spatial resolution of Chandra and in particular while planetary missions are making in situ measurements of solar wind and local conditions.

Type: Article
Title: X-ray studies of solar system objects: Past, present, and the next decade
Open access status: An open access version is available from UCL Discovery
DOI: 10.1002/asna.201713329
Publisher version: http://doi.org/10.1002/asna.201713329
Language: English
Additional information: This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: Solar system: general;X-rays: individual (solar system targets)
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/1569540
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