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Reply to comment by H. Hasegawa on "evolution of Kelvin-Helmholtz activity on the dusk flank magnetopause"

dc.contributor.authorFoullon, Claire
dc.contributor.authorFarrugia, Charles J.
dc.contributor.authorFazakerley, Andrew
dc.contributor.authorOwen, Christopher J.
dc.contributor.authorGratton, F.T.
dc.contributor.authorTorbert, R.B.
dc.date.accessioned2013-08-21T15:43:20Z
dc.date.issued2009
dc.identifier.citationVol. 114 (A10), article A10201en_GB
dc.identifier.doi10.1029/2009JA014444
dc.identifier.urihttp://hdl.handle.net/10871/12741
dc.language.isoenen_GB
dc.publisherAmerican Geophysical Union (AGU)en_GB
dc.relation.urlhttp://dx.doi.org/10.1029/2009JA014444en_GB
dc.titleReply to comment by H. Hasegawa on "evolution of Kelvin-Helmholtz activity on the dusk flank magnetopause"en_GB
dc.typeArticleen_GB
dc.date.available2013-08-21T15:43:20Z
dc.descriptionCopyright © 2009 American Geophysical Union (AGU)en_GB
dc.descriptionThis is a commentary on DOI:10.1029/2008JA013887en_GB
dc.identifier.eissn2169-9402
dc.identifier.journalJournal of Geophysical Research: Space Physicsen_GB


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