B.V. Jackson , H-S Yu , P.P. Hick, A. Buffington, J.M. Clover

1. B.V. Jackson, H-S Yu, P.P. Hick, A. Buffington, J.M. Clover Center for Astrophysics and Space Sciences, University of California at San Diego, LaJolla, CA, USA Munetoshi Tokumaru Solar-Terrestrial Environment Laboratory, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8601, Japan Masayoshi http://ips.ucsd.edu/

2. DATA STELab Interplanetary Scintillation (IPS) Heliospheric Analyses IPS line-of-sight response 3,432 m2 STELab IPS array in Toyokawa, Japan STELab IPS array systems

3. Heliospheric 3-D Reconstruction Jackson, B.V., et al., 2010, Adv. in Geosciences, 21, 339 The outward-flowing solar wind structure follows very specific physics as it moves outward from the Sun LOS Weighting

4. Heliospheric 3-D Reconstruction Jackson, B.V., et al., 2010, Adv. in Geosciences, 21, 339. Line of sight “crossed” components on a reference surface. Projections on the reference surface are shown. These weighted components are inverted to provide the time-dependent tomographic reconstruction. 13 July 2000 14 July 2000

5. IPS C.A.T. Analysis Jackson, B.V., et al., 2002, Solar Wind 10, 31 Bastille Day Event 14 July 2000 IPS Density Remote View

6. IPS C.A.T. Analysis Jackson, B.V., et al., 2002, Solar Wind 10, 31 Bastille Day Event 14 July 2000 IPS Density Ecliptic Cut

7. IPS C.A.T. Analysis Jackson, B.V., et al., 2002, Solar Wind 10, 31 Bastille Day Event 14 July 2000 IPS Velocity Ecliptic Cut

8. IPS C.A.T. Analysis Jackson, B.V., et al., 2002, Solar Wind 10, 31 Bastille Day Event 14 July 2000 IPS Density Meridional Cut IPS Density LOS X-ing Meridional Cut

9. Poster 087 THE 3D GLOBAL FORECAST OF INNER HELIOSPHERE SOLAR WIND PARAMETERS FROM REMOTELY-SENSED IPS DATA  Bernard V. Jackson1, John M. Clover1,P. Paul Hick1, Hsiu-Shan Yu1, Andrew Buffington1, and Munetoshi Tokumaru2 1CASS/UCSD, 2STELab, Nagoya University, Japan Interplanetary Scintillation (IPS) UCSD “Real-Time” Forecast UCSD Forecast Webpage  Aftcast Density New STELab radio array at Toyokawa (year-round operation) http//:ips.ucsd.edu Aftcast http://iswa.ccmc.gsfc.nasa.gov:8080/IswaSystemWebApp/index. jsp? Velocity  June 08 20 UT June 08 23 UT CCMC “Real-Time” Forecast July 14 0 UT

10. A 3D RECONSTRUCTED GLOBAL SOLAR WIND BOUNDARY FROM REMOTE-SENSING IPS DATA Poster 147 Hsiu-Shan Yu1, B.V. Jackson1, P.P. Hick1, A. Buffington1, J.M. Clover1, Munetoshi Tokumaru2, and Lan Jian3,4 1CASS/UCSD, 2STELab, Nagoya University, Japan, 3NASA GSFC, 4University of Maryland Time-Dependent Boundary at 0.25AU in Inertial Heliographic Coordinates (IHG) Toyokawa radio array of the Solar-Terrestrial Environment Laboratory (STELab), Japan LASCO C2 on 2011/11/09 CME to Southeast CME to Northeast CME to Southeast

11. The Solar Mass Ejection Imager (SMEI) Jackson, B.V., et al., 2004, Solar Phys., 225, 177 Launch 6 January 2003 Sun C1 C2 C3 Sun 1 gigabyte/day; now ~4 terabytes Simultaneous images from the three SMEI cameras. A joint US Air Force - NASA Project

12. ASI & other instrumentation accommodation Jackson, B.V., et al., 2010, “Lessons”, Solar Phys., 265, 257-275. NASA “White Paper” “Whole sky” ASI