dc.date.accessioned | 2019-03-12T08:56:17Z | |
dc.date.available | 2019-03-12T08:56:17Z | |
dc.date.created | 2019-01-18T20:20:37Z | |
dc.date.issued | 2018 | |
dc.identifier.citation | Gunell, Herbert Goetz, Charlotte Simon Wedlund, Cyril Lindkvist, Jesper Hamrin, Maria Nilsson, Hans Llera, Kristie Eriksson, Anders Holmström, Mats . The infant bow shock: A new frontier at a weak activity comet. Astronomy and Astrophysics. 2018, 619:L2, 1-5 | |
dc.identifier.uri | http://hdl.handle.net/10852/67125 | |
dc.description.abstract | The bow shock is the first boundary the solar wind encounters as it approaches planets or comets. The Rosetta spacecraft was able to observe the formation of a bow shock by following comet 67P/Churyumov–Gerasimenko toward the Sun, through perihelion, and back outward again. The spacecraft crossed the newly formed bow shock several times during two periods a few months before and after perihelion; it observed an increase in magnetic field magnitude and oscillation amplitude, electron and proton heating at the shock, and the diminution of the solar wind further downstream. Rosetta observed a cometary bow shock in its infancy, a stage in its development not previously accessible to in situ measurements at comets and planets. | en_US |
dc.language | EN | |
dc.publisher | EDP Sciences | |
dc.title | The infant bow shock: A new frontier at a weak activity comet | en_US |
dc.type | Journal article | en_US |
dc.creator.author | Gunell, Herbert | |
dc.creator.author | Goetz, Charlotte | |
dc.creator.author | Simon Wedlund, Cyril | |
dc.creator.author | Lindkvist, Jesper | |
dc.creator.author | Hamrin, Maria | |
dc.creator.author | Nilsson, Hans | |
dc.creator.author | Llera, Kristie | |
dc.creator.author | Eriksson, Anders | |
dc.creator.author | Holmström, Mats | |
cristin.unitcode | 185,15,4,70 | |
cristin.unitname | Plasma- og romfysikk | |
cristin.ispublished | true | |
cristin.fulltext | original | |
cristin.qualitycode | 2 | |
dc.identifier.cristin | 1660719 | |
dc.identifier.bibliographiccitation | info:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Astronomy and Astrophysics&rft.volume=619:L2&rft.spage=1&rft.date=2018 | |
dc.identifier.jtitle | Astronomy and Astrophysics | |
dc.identifier.volume | 619:L2 | |
dc.identifier.startpage | 1 | |
dc.identifier.endpage | 5 | |
dc.identifier.doi | http://dx.doi.org/10.1051/0004-6361/201834225 | |
dc.identifier.urn | URN:NBN:no-70315 | |
dc.type.document | Tidsskriftartikkel | en_US |
dc.type.peerreviewed | Peer reviewed | |
dc.source.issn | 0004-6361 | |
dc.identifier.fulltext | Fulltext https://www.duo.uio.no/bitstream/handle/10852/67125/1/aa34225-18.pdf | |
dc.type.version | PublishedVersion | |
dc.relation.project | NFR/240000 | |