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Predicting Solar Magnetic Field at Earth Dusan Odstrcil George Mason University & NASA/GSFC/Space Weather Laboratory MURI/NADIR Workshop Boulder, CO October 27- 28, 2010

Predicting Solar Magnetic Field at Earth

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Predicting Solar Magnetic Field at Earth. Dusan Odstrcil George Mason University & NASA/GSFC/Space Weather Laboratory. MURI/NADIR Workshop Boulder, CO October 27-28, 2010. Background Solar Wind by FR Coronal Maps. MAS and WSA coronal FR maps provide Br only - PowerPoint PPT Presentation

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Page 1: Predicting Solar Magnetic Field at Earth

Predicting Solar Magnetic Field at Earth

Dusan OdstrcilGeorge Mason University & NASA/GSFC/Space Weather Laboratory

MURI/NADIR Workshop Boulder, CO October 27-28, 2010

Page 2: Predicting Solar Magnetic Field at Earth

Background Solar Wind by FR Coronal Maps

MAS and WSA coronal FR maps provide Br only

ENLIL introduces Bphi at the inner boundary

Initially Btheta = 0; weak Bz by stream interaction

and seasonal effect

Page 3: Predicting Solar Magnetic Field at Earth

Bz in Simulations with FR Maps

Page 4: Predicting Solar Magnetic Field at Earth

Transient Disturbances

Modeling of the origin of CMEs is still in the research phases and it is not expected that real events can be routinely simulated in near future. Therefore, we have developed an intermediate modeling system which uses the WSA coronal maps, fitted coronagraph observations, specifies 3D ejecta, and drives 3D numerical code ENLIL.

Page 5: Predicting Solar Magnetic Field at Earth

IMF Draped by an ICME

Page 6: Predicting Solar Magnetic Field at Earth

“External” Bz Periods – Shock Compression

Shock to north, positive IMF: + Shock to north, negative IMF: -

Shock to south, positive IMF: - Shock to south, negative IMF: +

Page 7: Predicting Solar Magnetic Field at Earth

“External” Bz Periods – ICME Draping

Above ICME center, positive IMF: - + Above ICME center, negative IMF: + -

Below ICME center, positive IMF: + - Below ICME center, negative IMF: - +

Page 8: Predicting Solar Magnetic Field at Earth

Bz in Simulations with FR Maps and Cone

Page 9: Predicting Solar Magnetic Field at Earth

Bz in Simulations with FR Maps and Cone

Page 10: Predicting Solar Magnetic Field at Earth

May 12, 1997 – Interplanetary CME

MAS coronal model (PSI) ENLIL heliospheric model (GMU-NASA /GSFC)

Self-consistent end-to-end numerical simulation of space weather event(NSF/CISM effort in progress)

Page 11: Predicting Solar Magnetic Field at Earth

2008 April 26 CME with Rope Model

( Thernisien et al., 2009 ) ( WSA-1.6-GONG-CR2069 )

Page 12: Predicting Solar Magnetic Field at Earth

Launching Flux-Rope-Like Structure (2005-05-13)

Page 13: Predicting Solar Magnetic Field at Earth

Flux-Rope-Like Structure – Hydrodynamic

Page 14: Predicting Solar Magnetic Field at Earth

Flux-Rope-Like Structure – With 2D Magnetic Field

Page 15: Predicting Solar Magnetic Field at Earth

High-Resolution ICME Simulation – HD

Page 16: Predicting Solar Magnetic Field at Earth

High-Resolution Simulation

Page 17: Predicting Solar Magnetic Field at Earth

Conclusion

Solar Wind – Fully-automatic forecasting (Weak Bz events only)

ICMEs/fitted coronagraph observations – Semi-automatic forecasting (Moderate Bz by draping and shock compression)

ICMEs/self-consistent eruption– In active research (strong Bz)

ICMEs/semi-empirical flux ropes – Semi-automatic forecasting might ne possible (strong Bz)