Comment on “Comment on the abundances of rotational and tangential discontinuities in the solar wind” by M. Neugebauer

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dc.contributor.authorTsurutani, B.T.
dc.contributor.authorLakhina, G.S.
dc.contributor.authorVerkhoglyadova, O.P.
dc.contributor.authorEcher, Ezequiel
dc.contributor.authorGuarnieri, Fernando L.
dc.date.accessioned2015-09-08T08:54:05Z
dc.date.accessioned2021-02-12T09:28:40Z
dc.date.available2015-09-08T08:54:05Z
dc.date.available2021-02-12T09:28:40Z
dc.date.issued2007
dc.identifier.accession090849
dc.identifier.citationJournal of Geophysical Research, v.112, A03101, 2007, doi: 10.1029/2006JA011973en_US
dc.identifier.urihttp://library.iigm.res.in:4000/handle/123456789/356
dc.language.isoenen_US
dc.subjectTangential discontinuitiesen_US
dc.subjectRotational discontinuitiesen_US
dc.subjectSolar winden_US
dc.titleComment on “Comment on the abundances of rotational and tangential discontinuities in the solar wind” by M. Neugebaueren_US
dc.typeArticleen_US

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