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Investigating Mercury’s environment with the two-spacecraft BepiColombo mission
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Milillo2020_Article_InvestigatingMercurySEnvironme.pdf | Published version | 8.21 MB | Adobe PDF | View/Open |
Title: | Investigating Mercury’s environment with the two-spacecraft BepiColombo mission |
Authors: | Milillo Fujimoto Murakami Benkhoff Zender Aizawa Dósa Griton Heyner Ho Imber Jia Karlsson Killen Laurenza Lindsay McKenna-Lawlor Mura Raines Rothery André Baumjohann Berezhnoy Bourdin Bunce Califano Deca De la Fuente Dong Grava Fatemi Henri Ivanovski Jackson James Kallio Kasaba Kilpua Kobayashi Langlais Leblanc Lhotka Mangano Martindale Massetti Masters, A Morooka Narita Oliveira Odstrcil Orsini Pelizzo Plainaki Plaschke Sahraoui Seki Slavin Vainio Wurz Barabash Carr, C Delcourt Glassmeier Grande Hirahara Huovelin Korablev Kojima Lichtenegger Livi Matsuoka Moissl Moncuquet Muinonen Quèmerais Saito Yagitani Yoshikawa Wahlund |
Item Type: | Journal Article |
Abstract: | The ESA-JAXA BepiColombo mission will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric dynamics at Mercury as well as their interactions with the solar wind, radiation, and interplanetary dust. Many scientific instruments onboard the two spacecraft will be completely, or partially devoted to study the near-space environment of Mercury as well as the complex processes that govern it. Many issues remain unsolved even after the MESSENGER mission that ended in 2015. The specific orbits of the two spacecraft, MPO and Mio, and the comprehensive scientific payload allow a wider range of scientific questions to be addressed than those that could be achieved by the individual instruments acting alone, or by previous missions. These joint observations are of key importance because many phenomena in Mercury’s environment are highly temporally and spatially variable. Examples of possible coordinated observations are described in this article, analysing the required geometrical conditions, pointing, resolutions and operation timing of different BepiColombo instruments sensors. |
Issue Date: | 14-Jul-2020 |
Date of Acceptance: | 22-Jun-2020 |
URI: | http://hdl.handle.net/10044/1/81061 |
DOI: | 10.1007/s11214-020-00712-8 |
ISSN: | 0038-6308 |
Publisher: | Springer Verlag |
Start Page: | 1 |
End Page: | 78 |
Journal / Book Title: | Space Science Reviews |
Volume: | 216 |
Copyright Statement: | © The Author(s) 2020. This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/. |
Sponsor/Funder: | The Royal Society Science and Technology Facilities Council |
Funder's Grant Number: | UF150547 ST/S006230/1 |
Keywords: | Astronomy & Astrophysics 0201 Astronomical and Space Sciences |
Publication Status: | Published |
Article Number: | 93 |
Online Publication Date: | 2020-07-14 |
Appears in Collections: | Space and Atmospheric Physics Physics Faculty of Natural Sciences |
This item is licensed under a Creative Commons License