Using In Situ and Remote Sensing Data to Model the Plasma Flow throughout the Heliosphere
Tae K. Kim1, Nikolai V Pogorelov2, Charles Nickolos Arge3, Bernard V Jackson4, Igor Kryukov1, Periasamy K Manoharan5, Preethi Manoharan6, Derek Tropf7, Hsiu-Shan Yu8 and Gary Paul Zank9, (1)University of Alabama in Huntsville, CSPAR, Huntsville, AL, United States, (2)University of Alabama in Huntsville, Department of Space Science, Huntsville, AL, United States, (3)Air Force Research Laboratory Kirtland AFB, Kirtland AFB, NM, United States, (4)University of California, San Diego, Astronomy and Astrophysics, La Jolla, CA, United States, (5)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States, (6)University of Alabama in Huntsville, Huntsville, AL, United States, (7)NASA Jet Propulsion Laboratory, Washington, DC, United States, (8)University of California San Diego, Center for Astrophysics and Space Science, La Jolla, CA, United States, (9)University of Alabama in Huntsville, Space Science, Huntsville, AL, United States
