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Statistical properties of coronal hole rotation rates: are they linked to solar interiors?

dc.contributor.authorBagahvili, S.R.
dc.contributor.authorShergelashvili, B.M.
dc.contributor.authorJaparidze, D.R
dc.contributor.authorChargeishvili, B.B.
dc.contributor.authorKosovichev, A.G.
dc.contributor.authorKukhianidze, V.
dc.contributor.authorRamishvili, G.
dc.contributor.authorZaqarashvili, T.V.
dc.contributor.authorPoedts, S.
dc.contributor.authorKhodachenko, M.L.
dc.contributor.authorDe Causmaecker, P.
dc.date.accessioned2021-10-24T02:54:22Z
dc.date.available2021-10-24T02:54:22Z
dc.date.issued2017
dc.identifier.issn0004-6361
dc.identifier.urihttps://imec-publications.be/handle/20.500.12860/27786
dc.sourceIIOimport
dc.titleStatistical properties of coronal hole rotation rates: are they linked to solar interiors?
dc.typeJournal article
dc.date.embargo9999-12-31
dc.source.peerreviewyes
dc.source.beginpageA134
dc.source.journalAstronomy & Astrophysics
dc.source.volume603
dc.identifier.urlhttps://doi.org/10.1051/0004-6361/201630377
imec.availabilityPublished - open access


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