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Interaction of the solar wind with comets: a Rosetta perspective
The Rosetta mission provides an unprecedented possibility to study the interaction of comets with the solar wind. As the spacecraft accompanies comet 67P/Churyumov–Gerasimenko from its very low-activity stage through its perihelion phase, the physics of mass loading is witnessed for various activity...
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Formato: | Online Artículo Texto |
Lenguaje: | English |
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The Royal Society Publishing
2017
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Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5454225/ https://www.ncbi.nlm.nih.gov/pubmed/28554976 http://dx.doi.org/10.1098/rsta.2016.0256 |
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author | Glassmeier, Karl-Heinz |
author_facet | Glassmeier, Karl-Heinz |
author_sort | Glassmeier, Karl-Heinz |
collection | PubMed |
description | The Rosetta mission provides an unprecedented possibility to study the interaction of comets with the solar wind. As the spacecraft accompanies comet 67P/Churyumov–Gerasimenko from its very low-activity stage through its perihelion phase, the physics of mass loading is witnessed for various activity levels of the nucleus. While observations at other comets provided snapshots of the interaction region and its various plasma boundaries, Rosetta observations allow a detailed study of the temporal evolution of the innermost cometary magnetosphere. Owing to the short passage time of the solar wind through the interaction region, plasma instabilities such as ring--beam and non-gyrotropic instabilities are of less importance during the early life of the magnetosphere. Large-amplitude ultra-low-frequency (ULF) waves, the ‘singing’ of the comet, is probably due to a modified ion Weibel instability. This instability drives a cross-field current of implanted cometary ions unstable. The initial pick-up of these ions causes a major deflection of the solar wind protons. Proton deflection, cross-field current and the instability induce a threefold structure of the innermost interaction region with the characteristic Mach cone and Whistler wings as stationary interaction signatures as well as the ULF waves representing the dynamic aspect of the interaction. This article is part of the themed issue ‘Cometary science after Rosetta’. |
format | Online Article Text |
id | pubmed-5454225 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2017 |
publisher | The Royal Society Publishing |
record_format | MEDLINE/PubMed |
spelling | pubmed-54542252017-06-05 Interaction of the solar wind with comets: a Rosetta perspective Glassmeier, Karl-Heinz Philos Trans A Math Phys Eng Sci Articles The Rosetta mission provides an unprecedented possibility to study the interaction of comets with the solar wind. As the spacecraft accompanies comet 67P/Churyumov–Gerasimenko from its very low-activity stage through its perihelion phase, the physics of mass loading is witnessed for various activity levels of the nucleus. While observations at other comets provided snapshots of the interaction region and its various plasma boundaries, Rosetta observations allow a detailed study of the temporal evolution of the innermost cometary magnetosphere. Owing to the short passage time of the solar wind through the interaction region, plasma instabilities such as ring--beam and non-gyrotropic instabilities are of less importance during the early life of the magnetosphere. Large-amplitude ultra-low-frequency (ULF) waves, the ‘singing’ of the comet, is probably due to a modified ion Weibel instability. This instability drives a cross-field current of implanted cometary ions unstable. The initial pick-up of these ions causes a major deflection of the solar wind protons. Proton deflection, cross-field current and the instability induce a threefold structure of the innermost interaction region with the characteristic Mach cone and Whistler wings as stationary interaction signatures as well as the ULF waves representing the dynamic aspect of the interaction. This article is part of the themed issue ‘Cometary science after Rosetta’. The Royal Society Publishing 2017-07-13 2017-05-29 /pmc/articles/PMC5454225/ /pubmed/28554976 http://dx.doi.org/10.1098/rsta.2016.0256 Text en © 2017 The Authors. http://creativecommons.org/licenses/by/4.0/ Published by the Royal Society under the terms of the Creative Commons Attribution License http://creativecommons.org/licenses/by/4.0/, which permits unrestricted use, provided the original author and source are credited. |
spellingShingle | Articles Glassmeier, Karl-Heinz Interaction of the solar wind with comets: a Rosetta perspective |
title | Interaction of the solar wind with comets: a Rosetta perspective |
title_full | Interaction of the solar wind with comets: a Rosetta perspective |
title_fullStr | Interaction of the solar wind with comets: a Rosetta perspective |
title_full_unstemmed | Interaction of the solar wind with comets: a Rosetta perspective |
title_short | Interaction of the solar wind with comets: a Rosetta perspective |
title_sort | interaction of the solar wind with comets: a rosetta perspective |
topic | Articles |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5454225/ https://www.ncbi.nlm.nih.gov/pubmed/28554976 http://dx.doi.org/10.1098/rsta.2016.0256 |
work_keys_str_mv | AT glassmeierkarlheinz interactionofthesolarwindwithcometsarosettaperspective |