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dc.contributor.authorVerbeeck, C.*
dc.contributor.authorHiggins, P.A.*
dc.contributor.authorColak, Tufan*
dc.contributor.authorWatson, F.T.*
dc.contributor.authorDelouille, V.*
dc.contributor.authorMampaey, B.*
dc.contributor.authorQahwaji, Rami S.R.*
dc.date.accessioned2016-01-18T15:01:07Z
dc.date.available2016-01-18T15:01:07Z
dc.date.issued2013-03
dc.identifier.citationVerbeeck C, Higgins PA, Colak T, Watson FT, Delouille V, Mampaey B and Qahwaji RSR (2013) A multi-wavelength analysis of active regions and sunspots by comparison of automatic detection algortihms. Solar Physics. 283(1): 67-95.en_US
dc.identifier.urihttp://hdl.handle.net/10454/7682
dc.descriptionYesen_US
dc.description.abstractThe launch of the Solar Dynamics Observatory (SDO) in early 2010 has provided the solar physics community with the most detailed view of the Sun to date. However, this presents new challenges for the analysis of solar data. Currently, SDO sends over 1 terabyte of data per day back to Earth and methods for fast and reliable analysis are more important than ever. This article details four algorithms developed separately at the Universities of Bradford and Glasgow, the Royal Observatory of Belgium and Trinity College Dublin for the purposes of automated detection of solar active regions (ARs) and sunspots at different levels of the solar atmosphere.en_US
dc.language.isoenen_US
dc.relation.isreferencedbyhttp://dx.doi.org/10.1007/s11207-011-9859-6en_US
dc.rights(c) 2013 Springer Netherlands. Full-text reproduced in accordance with the publisher's self-archiving policy.en_US
dc.subjectActive regions; Magnetic fields; Coronal structures; Sunspotsen_US
dc.titleA multi-wavelength analysis of active regions and sunspots by comparison of automatic detection algorithmsen_US
dc.status.refereedYesen_US
dc.typeArticleen_US
dc.type.versionAccepted Manuscripten_US
refterms.dateFOA2018-07-25T13:53:54Z


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