Helioseismology in Space Weather - National Solar Observatory

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Input DataSolarMagnetogramDataIncorporating Far-Side Observationsinto ADAPTIntelligent FrontEnd !Import & SelectDataforData AssimilatorADAPTInitial ConditionsData AssimilatorForecast Step:use the WHmodel tocalculateforecastModeling / ForecastingApplicationsImprovedSolar SynopticMapsCoronal &Solar WindModelsWSA+ENLILMagneticFieldVarianceAnalysis Step:combineobservations withforecastFar-side mapPolarity+ErrorEstimationAssimilation ResultsGlobalMagnetic FieldWSA-ENLILSolar WindDiagram of the general data flow and processing of ADAPT: the Intelligent Front End imports and selects the bestavailable magnetogram data, along with estimated uncertainties, to be assimilated by the ensemble least-squares (EnLS)method with the latest WH flux transport map of the global solar magnetic field. These maps are then used as input forcoronal and solar wind models, e.g., WSA-ENLIL (Odstrcil et al. , 2005) .
ADAPT: Photospheric Field(Before & After Far-Side Active Region Insertion)Large, GONGdetected far-sideactive regioninserted into theADAPT map on July1, 2010June 30, 2010Without Active RegionInsertedJuly 1, 2010With Active RegionInsertedArge, N. et al (Solar Wind 13 presentation, June 2012)
Page 1: Helioseismology in Space WeatherIre
Page 4 and 5: Helioseismology of Active RegionTim
Page 6 and 7: Helioseismology of Active RegionsCo
Page 8 and 9: Current Far-side MapsMagnetic field
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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