Publication:

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

Date

2017
Journal article
Simple item page Full metadata Statistics
 
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.embargo9999-12-31
dc.date.issued2017
dc.identifier.issn0004-6361
dc.identifier.urihttps://imec-publications.be/handle/20.500.12860/27786
dc.identifier.urlhttps://doi.org/10.1051/0004-6361/201630377
dc.source.beginpageA134
dc.source.journalAstronomy & Astrophysics
dc.source.volume603
dc.title

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

dc.typeJournal article
dspace.entity.typePublication
Files

Original bundle

Name:
41083.pdf
Size:
388.45 KB
Format:
Adobe Portable Document Format
Download
Publication available in collections:
Articles