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Mass-loading of the solar wind at 67P/Churyumov-Gerasimenko: Observations and modelling
Luleå tekniska universitet, Institutionen för system- och rymdteknik, Rymdteknik.ORCID-id: 0000-0003-0177-510X
Swedish Institute of Space Physics, Kiruna.
Luleå tekniska universitet, Institutionen för system- och rymdteknik, Rymdteknik.
Swedish Institute of Space Physics, Kiruna.
Vise andre og tillknytning
Rekke forfattare: 72016 (engelsk)Inngår i: Astronomy and Astrophysics, ISSN 0004-6361, E-ISSN 1432-0746, Vol. 596, artikkel-id A42Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

Context. The first long-term in-situ observation of the plasma environment in the vicinity of a comet, as provided by the European Rosetta spacecraft. Aims. Here we offer characterisation of the solar wind flow near 67P/Churyumov-Gerasimenko (67P) and its long term evolution during low nucleus activity. We also aim to quantify and interpret the deflection and deceleration of the flow expected from ionization of neutral cometary particles within the undisturbed solar wind. Methods. We have analysed in situ ion and magnetic field data and combined this with hybrid modeling of the interaction between the solar wind and the comet atmosphere. Results. The solar wind deflection is increasing with decreasing heliocentric distances, and exhibits very little deceleration. This is seen both in observations and in modeled solar wind protons. According to our model, energy and momentum are transferred from the solar wind to the coma in a single region, centered on the nucleus, with a size in the order of 1000 km. This interaction affects, over larger scales, the downstream modeled solar wind flow. The energy gained by the cometary ions is a small fraction of the energy available in the solar wind. Conclusions. The deflection of the solar wind is the strongest and clearest signature of the mass-loading for a small, low-activity comet, whereas there is little deceleration of the solar wind

sted, utgiver, år, opplag, sider
2016. Vol. 596, artikkel-id A42
HSV kategori
Forskningsprogram
Atmosfärsvetenskap
Identifikatorer
URN: urn:nbn:se:ltu:diva-61146DOI: 10.1051/0004-6361/201628797ISI: 000390797900062Scopus ID: 2-s2.0-85000443624OAI: oai:DiVA.org:ltu-61146DiVA, id: diva2:1057750
Merknad

Validerad; 2017; Nivå 2; 2016-12-19 (andbra)

Tilgjengelig fra: 2016-12-19 Laget: 2016-12-19 Sist oppdatert: 2018-07-10bibliografisk kontrollert
Inngår i avhandling
1. The dynamics of the solar wind in the atmosphere of comet 67P/Churyumov-Gerasimenko
Åpne denne publikasjonen i ny fane eller vindu >>The dynamics of the solar wind in the atmosphere of comet 67P/Churyumov-Gerasimenko
2018 (engelsk)Doktoravhandling, med artikler (Annet vitenskapelig)
sted, utgiver, år, opplag, sider
Luleå University of Technology, 2018
Serie
Doctoral thesis / Luleå University of Technology 1 jan 1997 → …, ISSN 1402-1544
HSV kategori
Forskningsprogram
Atmosfärsvetenskap
Identifikatorer
urn:nbn:se:ltu:diva-68785 (URN)978-91-7790-156-3 (ISBN)978-91-7790-157-0 (ISBN)
Disputas
2018-10-12, Aula, IRF, Kiruna, 08:16 (engelsk)
Opponent
Veileder
Tilgjengelig fra: 2018-05-21 Laget: 2018-05-18 Sist oppdatert: 2018-05-21bibliografisk kontrollert

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