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dc.contributor.authorBamford, R. A.
dc.contributor.authorAlves, E. P.
dc.contributor.authorCruz, F.
dc.contributor.authorKellett, B. J.
dc.contributor.authorFonsesca, R. A.
dc.contributor.authorSilva, L. O.
dc.contributor.authorTrines, R. M. G. M.
dc.contributor.authorHalekas, J. S.
dc.contributor.authorKamer, G.
dc.contributor.authorHarnett, E.
dc.contributor.authorCairns, Robert Alan
dc.contributor.authorBingham, R.
dc.date.accessioned2017-06-22T16:30:08Z
dc.date.available2017-06-22T16:30:08Z
dc.date.issued2016-10-18
dc.identifier.citationBamford , R A , Alves , E P , Cruz , F , Kellett , B J , Fonsesca , R A , Silva , L O , Trines , R M G M , Halekas , J S , Kamer , G , Harnett , E , Cairns , R A & Bingham , R 2016 , ' 3D pic simulations of collisionless shocks at lunar magnetic anomalies and their role in forming lunar swirls ' Astrophysical Journal , vol. 830 , no. 2 . https://doi.org/10.3847/0004-637X/830/2/146en
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 250299191
dc.identifier.otherPURE UUID: 0cfc4674-f71c-4a6c-92b5-d07a65f0c4c1
dc.identifier.otherScopus: 84993971772
dc.identifier.otherWOS: 000400471800013
dc.identifier.urihttp://hdl.handle.net/10023/11067
dc.descriptionThe authors would like to thank the Science and Technology Facilities Council for fundamental physics and computing resources that were provided by funding from STFC’s Scientific Computing Department, and would like to thank the European Research Council (ERC 2010 AdG Grant 267841) and FCT (Portugal) grants SFRH/BD/75558/2010 for support.en
dc.description.abstractInvestigation of the lunar crustal magnetic anomalies offers a comprehensive long-term data set of observations of small-scale magnetic fields and their interaction with the solar wind. In this paper a review of the observations of lunar mini-magnetospheres is compared quantifiably with theoretical kinetic-scale plasma physics and 3D particle-in-cell simulations. The aim of this paper is to provide a complete picture of all the aspects of the phenomena and to show how the observations from all the different and international missions interrelate. The analysis shows that the simulations are consistent with the formation of miniature (smaller than the ion Larmor orbit) collisionless shocks and miniature magnetospheric cavities, which has not been demonstrated previously. The simulations reproduce the finesse and form of the differential proton patterns that are believed to be responsible for the creation of both the "lunar swirls" and "dark lanes." Using a mature plasma physics code like OSIRIS allows us, for the first time, to make a side-by-side comparison between model and space observations. This is shown for all of the key plasma parameters observed to date by spacecraft, including the spectral imaging data of the lunar swirls. The analysis of miniature magnetic structures offers insight into multi-scale mechanisms and kinetic-scale aspects of planetary magnetospheres.
dc.format.extent12
dc.language.isoeng
dc.relation.ispartofAstrophysical Journalen
dc.rights© 2016. The American Astronomical Society. All rights reserved. This work is made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at: https://dx.doi.org/10.3847/0004-637X/830/2/146en
dc.subjectAcceleration of particlesen
dc.subjectMoonen
dc.subjectMagnetic fieldsen
dc.subjectPlanets and satellites: magnetic fieldsen
dc.subjectPlasmasen
dc.subjectShock wavesen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectNDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.title3D pic simulations of collisionless shocks at lunar magnetic anomalies and their role in forming lunar swirlsen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.Applied Mathematicsen
dc.identifier.doihttps://doi.org/10.3847/0004-637X/830/2/146
dc.description.statusPeer revieweden
dc.identifier.urlhttp://adsabs.harvard.edu/abs/2016ApJ...830..146Ben
dc.identifier.urlhttp://strathprints.strath.ac.uk/id/eprint/59294en


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