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IPS Heliospheric Analyses (STELab)

IPS Heliospheric Analyses (STELab). DATA. IPS line-of-sight response. STELab IPS array near Mt. Fuji. STELab IPS array systems. Current STELab Toyokawa IPS System. New STELab IPS array in Toyokawa (3,432 m 2 array now operates well – year-round operation began in 2011).

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IPS Heliospheric Analyses (STELab)

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  1. IPS Heliospheric Analyses (STELab) DATA IPS line-of-sight response STELab IPS array near Mt. Fuji STELab IPS array systems

  2. Current STELab Toyokawa IPS System New STELab IPS array in Toyokawa (3,432 m2 array now operates well – year-round operation began in 2011)

  3. IPS line-of-sight response Jackson, B.V., et al., 2008, Adv. in Geosciences, 21, 339-360. Heliospheric C.A.T. analyses: example line-of-sight distribution for each sky location to form the source surface of the 3D reconstruction. STELab IPS 14 July 2000 13 July 2000

  4. IPS C.A.T. Analysis Jackson, B.V., et al., 2002, Solar Wind 10, 31 Bastille Day Event 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

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

  7. 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

  8. Zhao, X. P. and Hoeksema, J. T., 1995, J. Geophys. Res., 100 (A1), 19. http://ips.ucsd.edu/ Magnetic Field Extrapolation • Inner region: the CSSS model calculates the magnetic field usingphotospheric measurements and a horizontal current model. 2. Middle region: the CSSS model opens the field lines. In the outer region. 3. Outer region: the UCSD tomography convects the magnetic field along velocity flow lines. Dunn et al., 2005, Solar Physics 227: 339–353. Jackson, B.V., et al., 2012, Adv. in Geosciences, 30, 93-115.

  9. IPS C.A.T. Analysis Dunn, T.J., et al., 2005, Solar Phys., 227, 339 Potential field modeling added IPS Density Remote View

  10. Jackson, B.V., et al., 2010,Solar Phys., 265, 245-256. IPS line-of-sight response Jackson, B.V., et al., 2010, Adv. in Geosciences, 21, 339-360. Jackson, B.V., et al., 2012,Solar Phys. published on-line. Heliospheric C.A.T. Analyses: example line-of-sight distribution for each sky location to form the source surface of the 3D reconstruction. Innovation STELab IPS * 13 July 2000 Inclusion of in-situ measurements into the 3D-reconstructions

  11. Heliospheric 3D-reconstructions Jackson, B.V., et al., 2010,Solar Phys., 265, 245-256. Innovation Innovation Inclusion of in-situ measurements into the 3D-reconstructions Jackson, B.V., et al., 2008, Adv. in Geosciences, (in press).

  12. Heliospheric 3D-reconstructions Jackson, B.V., et al., 2010,Solar Phys., 265, 245-256. Jackson, B.V., et al., 2011, Adv. in Geosciences, 30, 93-115. Forecast Jackson, B.V., et al., 2012,Solar Phys. published on-line. Density Forecast Forecast Inclusion of in-situ measurements into the 3D-reconstructions Forecasts work better if the values match up to the present. Velocity Forecast

  13. Heliospheric 3D-reconstructions Jackson, B.V., et al., 2010,Solar Phys., 265, 245-256. Jackson, B.V., et al., 2011, Adv. in Geosciences, 30, 93-115. Forecast Jackson, B.V., et al., 2012,Solar Phys. published on-line. Density Density Forecast Inclusion of in-situ measurements into the 3D-reconstructions Forecasts work better if the values match up to the present. Velocity Velocity Forecast

  14. Jackson, B.V., et al., 2011, Adv. in Geosciences, 30, 93-115. http://ips.ucsd.edu/ UCSD Web pages UCSD IPS forecasts Web Analysis Runs Automatically Using Linux on a P.C.

  15. Other and Potential Future IPS systems MEXART (Mexico) KSWC (South Korea) Dedicated IPS 700 m2 327 MHz IPS radio 32 tile array, Jeju Island Dedicated IPS IPS 9,600 m2 140 MHz IPS radio array near Michoacan, Mexico MWA (Western Australia) LOFAR (Western Europe) (32 tiles are now operating. The full array 128 tiles can obtain some IPS data.) (Some parts of the system are now operating - Richard Fallows, Mario Bisi are involved. IPS/FR tests are ongoing.)

  16. Oberoi and Lonsdale, 2012, Radio Science, 47, RS0K08, doi:10.1029/2012RS004992. Faraday rotation signals at low frequency ‗‗Φ = λ2 ∫ neB•ds From Oberoi and Lonsdale

  17. Future Jackson, B.V., et al., 2008,URAS Workshop ‗‗Φ = λ2 ∫ neB•ds Jensen, E.A., et al., 2010,Solar Phys., 265, 31 Faraday rotation tomography Background Field, 3D UCSD Density Background Field, 3D UCSD Density, Mulligan “Can”

  18. Summary: The Future is here: • Forecasts with the IPS data (this has worked with STELab data for about 12 years). • Forecasts in real-time work better now with the inclusion of in-situ data (has been available since spring, 2011) These new innovations and the inclusion of other world IPS data sets make the technique a competitive way to measure velocities and densities. • FR inversion to obtain vector fields may work, but needs to be incorporated with a robust method of determining density to back out accurate vector magnetic fields remotely.

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