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Dynamics of Coronal Bright Points as Seen by Sun Watcher Using Active Pixel System Detector and Image Processing (SWAP), Atmospheric Imaging Assembly (AIA), and Helioseismic and Magnetic Imager (HMI)

dc.contributor.authorChandrashekhar K.
dc.contributor.authorKrishna Prasad S.
dc.contributor.authorBanerjee D.
dc.contributor.authorRavindra B.
dc.contributor.authorSeaton D. B.
dc.date8/2013
dc.date.accessioned2016-04-13T10:05:11Z
dc.date.available2016-04-13T10:05:11Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3762
dc.descriptionhttp://esoads.eso.org/abs/2013SoPh..286..125C
dc.languageeng
dc.rightsRestricted Access
dc.titleDynamics of Coronal Bright Points as Seen by Sun Watcher Using Active Pixel System Detector and Image Processing (SWAP), Atmospheric Imaging Assembly (AIA), and Helioseismic and Magnetic Imager (HMI)
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleSolar Physics
dc.source.volume286
dc.source.page125
Orfeo.peerreviewedYes
dc.identifier.doi10.1007/s11207-012-0046-1
dc.identifier.urlhttp://esoads.eso.org/abs/2013SoPh..286..125C
dc.source.editorSPRINGER


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