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3D-MHD Models Driven by IPS

3D-MHD Models Driven by IPS. H.-S. Yu Center for Astrophysics and Space Sciences, University of California at San Diego, LaJolla, CA, USA. http://smei.ucsd.edu/ http://ips.ucsd.edu/ ftp://cass185.ucsd.edu/data/IPSBD_Real_Time/. IPS Time-Dependent 3D Tomographic Reconstructions.

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3D-MHD Models Driven by IPS

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  1. 3D-MHD Models Driven by IPS H.-S. Yu Center for Astrophysics and Space Sciences, University of California at San Diego, LaJolla, CA, USA http://smei.ucsd.edu/ http://ips.ucsd.edu/ ftp://cass185.ucsd.edu/data/IPSBD_Real_Time/

  2. IPS Time-Dependent 3D Tomographic Reconstructions

  3. 2011/11/09 CME LASCO C2 COR2 B

  4. 2011/11/09 CME (Forecast) LASCO C2 IPS Fish-eye map of Event

  5. 2011/11/09 CME (Forecast) LASCO C2 IPS Remote-Observer View

  6. IPS C.A.T. Analysis Jackson, B.V., et al., 2008, Adv. in Geosciences, 21, 339. Jackson, B.V., et al., 2013, Solar Phys. 285, 151. (Forecast) 2011/11/09 CME Density Ecliptic Cut Density Meridional Cut

  7. IPS C.A.T. Analysis Jackson, B.V., et al., 2008, Adv. in Geosciences, 21, 339. Jackson, B.V., et al., 2013, Solar Phys. 285, 151. (Forecast) (Forecast) 2011/11/09 CME Forecast Density Ecliptic Cut Density Forecast at 1AU

  8. IPS C.A.T. Analysis Jackson, B.V., et al., 2008, Adv. in Geosciences, 21, 339. Jackson, B.V., et al., 2013, Solar Phys. 285, 151. (Forecast) (Forecast) 2011/11/09 CME Forecast Velocity Ecliptic Cut Velocity Forecast at 1AU

  9. Global Solar Wind Boundary Evaluating the 3D reconstruction at a given spherical radius provides a “global solar wind lower boundary” which can then be extrapolated outward by 3D-MHD models. Results of this extrapolation can be compared with in-situ measurements as a “ground truth” verification of this technique.

  10. Time-Dependent Boundary in Inertial Heliographic Coordinates (IHG)

  11. Time-Dependent Boundary in Inertial Heliographic Coordinates (IHG)

  12. 3D-MHD Models Driven by IPS MS-FLUKSS 3D-MHD modeling from a 0.25AU 3D time-dependent IPS tomography boundary. (Kim, T. K., 2012, AIP Conference Proc. 1500, pp. 140-146.) Measurements at Earth

  13. Time-Dependent Boundary in Heliographic Coordinates (Earth-entered) ftp://cass185.ucsd.edu/data/IPSBD_Real_Time/

  14. Time-Dependent Boundary in Heliographic Coordinates (Earth-entered) ftp://cass185.ucsd.edu/data/IPSBD_Real_Time/

  15. 3D-MHD Models Driven by IPS-ENLIL Measurements at Earth Interesting Event

  16. ENLIL Model Drivers WSA Model MAS Model UCSD Model WSA Data MAS Data MAS Data UCSD Data In-Situ Data wsa2bc mas2bc mas2bc ucsd2bc coho2bc a3d2bc bnd.nc bnd.nc bnd.nc bnd.nc bnd.nc bnd.nc bnd.nc cone2bc ENLIL • Currently, there are three models (yellow) that can be used to drive ENLIL (green) • Computational system shares data sets (grey) and uses couplers (blue)

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