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dc.contributor.authorNilsson, H.
dc.contributor.authorBehar, E.
dc.contributor.authorBurch, J.L.
dc.contributor.authorCarr, C.M.
dc.contributor.authorEriksson, A.I.
dc.contributor.authorGlassmeier, K.‐H.
dc.contributor.authorHenri, P.
dc.contributor.authorGaland, M.
dc.contributor.authorGoetz, C.
dc.contributor.authorGunell, H.
dc.contributor.authorKarlsson, T.
dc.contributor.editor
dc.date2021
dc.date.accessioned2021-05-15T15:54:37Z
dc.date.available2021-05-15T15:54:37Z
dc.identifier.urihttps://orfeo.kbr.be/handle/internal/7761
dc.descriptionA magnetosphere may form around an object in a stellar wind either due to the intrinsic magnetic field of the object or stellar wind interaction with the ionosphere of the object. Comets represent the most variable magnetospheres in our solar system, and through the Rosetta mission we have had the chance to study the birth and evolution of a comet magnetosphere as the comet nucleus approached the Sun. We review the birth of the comet magnetosphere as observed at comet 67P Churyumov–Gerasimenko, the formation of plasma boundaries and how the solar wind–atmosphere interaction changes character as the cometary gas cloud and magnetosphere grow in size. Mass loading of the solar wind leads to an asymmetric deflection of the solar wind for low outgassing rates. With increasing activity a solar wind ion cavity forms. Intermittent shock‐like features were also observed. For intermediate outgassing rate a diamagnetic cavity is formed inside the solar wind ion cavity, thus well separated from the solar wind. The cometary plasma was typically very structured and variable. The region of the coma dense enough to have significant collisions forms a special region with different ion chemistry and plasma dynamics as compared to the outer collision‐free region.
dc.languageeng
dc.publisherWiley-American Geophysical Union, Hoboken, NJ, USA
dc.relation.ispartofseriesGeophysical Monograph Series
dc.titleBirth of a Magnetosphere
dc.typeBook chapter
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freecomet magnetosphere
dc.subject.freecomet nucleus
dc.subject.freecometary plasma boundaries
dc.subject.freeelectric fields
dc.subject.freeion chemistry
dc.subject.freeplasma dynamics
dc.subject.freeRosetta plasma observations
dc.subject.freesolar wind–atmosphere interaction
dc.source.titleMagnetospheres in the Solar System
dc.source.volume259
dc.source.page427-439
Orfeo.peerreviewedYes
dc.identifier.doi10.1002/9781119815624.ch27
dc.source.editorMaggiolo, R.
dc.source.editorAndré, N.
dc.source.editorHasegawa, H.
dc.source.editorWelling, D.T.
dc.source.editorZhang, Y.
dc.source.editorPaxton, L.J.


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