Helioseismology in Space Weather - National Solar Observatory

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Helioseismology of Active RegionTime distance: First seimic image of an active regionusing a local helioseismology technique (time-distance)Ambient Acoustic Imaging: Constructed outgoing intensitymap and phase-shift map at the surface and 10 Mm at 5mHzØ Chang, H.-K.,Chou, D.-Y.;Labonte, B. and the TONTeam, 1997, Nature, 389,825.Ø Chou, D.-Y., 2000, SolarPhysics, 192, 241Helioseismic holography: First seimic image of activeregions in the far side of the SunDuvall, T., D’Silva, S., Jefferies, S.M., Harvey,J.W. and Schou, 1996, Nature, 379, 235Lindsey, C. and Braun, D. C. 2000, Science, 287, 1799
Helioseismology of Active Regions16 oq Hill, F; 1988, ApJ,333,996q Patrón, J.; Hill, F.;Rhodes,E.J.,Jr.;Korzennik,S. G. andCacciani,A., 1995, ApJ, 455,746
Page 1: Helioseismology in Space WeatherIre
Page 6 and 7: Helioseismology of Active RegionsCo
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

Helioseismology in Space Weather - National Solar Observatory

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