Helioseismology in Space Weather - National Solar Observatory

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Helioseismology in Space Weather - National Solar Observatory

Helioseismology in Space Weather - National Solar Observatory

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Helioseismic Imag<strong>in</strong>g of the FarsidePhase of theCorrelation∫C( r,z,τ ) dtH ( r,z,t)H ( r,z,t + τ )=+−0 180 360Carr<strong>in</strong>gton Longitude (degrees)

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Numerical Simulations of Solar Magneto-Convection

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<strong>Helioseismology</strong> of Active RegionsCourtesy of R. Komm

Helioseismic Imag<strong>in</strong>g of the FarsidePhase of theCorrelation∫C( r,z,τ ) dtH ( r,z,t)H ( r,z,t + τ )=+−0 180 360Carr<strong>in</strong>gton Longitude (degrees)

Page 1: Helioseismology in Space WeatherIre
Page 4 and 5: Helioseismology of Active RegionTim
Page 8 and 9: Current Far-side MapsMagnetic field
Page 10 and 11: Input DataSolarMagnetogramDataIncor
Page 12 and 13: • WSA Coronalholes - Whitecontour
Page 14 and 15: F 10.7 Forecasting Using ADAPT(with
Page 16 and 17: Validation of far-side seismic maps
Page 18 and 19: Far-side seismic maps: Next Generat
Page 20 and 21: Flares and subsurface dynamicsTotal
Page 22 and 23: Emerging Active RegionsOriginal Pap
Page 24 and 25: Emerging Active RegionsBirch, A. et
Page 26 and 27: Emerging Active RegionsDeep focusin