Helioseismology in Space Weather - National Solar Observatory

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Flares and subsurface dynamicsTotal flareintensity of activeregions duringtheir diskpassage as afunction ofunsignedsubsurfacevorticity at 12Mm.Two-dimensionalhistogram of thenumber of activeregion as afunction ofunsignedmagnetic flux andunsignedsubsurfacevorticity at 12 Mm.Komm, R. and Hill, F. 2009, JGRA, 114
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Page 1: Helioseismology in Space WeatherIre
Page 4 and 5: Helioseismology of Active RegionTim
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Page 22 and 23: Emerging Active RegionsOriginal Pap
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Helioseismology in Space Weather - National Solar Observatory

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