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Fletcher, Lyndsay
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document
Detection and characterisation of the solar UV network
Abstract
WhenviewedatUVwavelengths(1600and1700 Angstroms)thereisanetworklikestructurevisibleuponthesolardisk,appearingprominentlyin activeregionsbutalsoformingtheboundarybetweengranulationcells. TheavailabilityofhighresolutiondatafromtheSolarDynamic Observatory (SDO) satellite allows us to examine this network in great detail. As such, this work uses several image processing techniques in an attempt to quantify whatpercentageofthesolardisk this'network'makes up, withcurrent resultssuggestingthatabout30%ofthediskisnetwork.Furtheranalysisof these results reveals a monthly fluctuation in the covering percentage and a correlation with the F10.7 flux. Our ongoing work tries to discern whether this variation and correlation has a component related to the network or is simply from the presence of active regions within the detection methods.