Helioseismology in Space Weather - National Solar Observatory
Helioseismology in Space Weather - National Solar Observatory
Helioseismology in Space Weather - National Solar Observatory
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Emerg<strong>in</strong>g Active RegionsHelioseismic holography is applied tosamples of the two populations (preemergenceand without emergence), eachsample hav<strong>in</strong>g over 100 members, whichwere selected to m<strong>in</strong>imize systematic bias,as described <strong>in</strong> Leka et al.Birch, A. et al, 2012, ApJ, 762We f<strong>in</strong>d that there are statistically significantsignatures (i.e., difference <strong>in</strong> the means of morethan a few standard errors) <strong>in</strong> the averagesubsurface flows and the apparent wave speed thatprecede the formation of an active region. Themeasurements here rule out spatially extendedflows of more than about 15 m/s <strong>in</strong> the top 20Mm below the photosphere over the course of theday preced<strong>in</strong>g the start of visible emergence.These measurements place strong constra<strong>in</strong>ts onmodels of active region formation.