An Iterative Interplanetary Scintillation (IPS) Analysis Using Time-dependent 3-D MHD Models as Kernels
Bernard V Jackson1, Hsiu-Shan Yu2, P. Paul Hick3, Andrew Buffington3, Dusan Odstrcil4, Tae K. Kim5, Nikolai V Pogorelov6, Munetoshi Tokumaru7, Mario Mark Bisi8, Jae Hun Kim9 and Jongyeon Yun10, (1)University of California, San Diego, Astronomy and Astrophysics, La Jolla, CA, United States, (2)University of California San Diego, Center for Astrophysics and Space Science, La Jolla, CA, United States, (3)University of California San Diego, Astronomy and Astrophysics, La Jolla, CA, United States, (4)George Mason University, Fairfax, United States, (5)The University of Alabama in Huntsville, CSPAR, Huntsville, AL, United States, (6)University of Alabama in Huntsville, Department of Space Science, Huntsville, AL, United States, (7)Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan, (8)STFC Rutherford Appleton Laboratory, RAL Space, Harwell Campus, Didcot, United Kingdom, (9)University of California Irvine, Irvine, CA, United States, (10)Space Environment Laboratory, 150-gil, Gangnam-gu, Seoul, Korea, Republic of (South)
