Potential Use of Observations of Interplanetary Scintillation (IPS) and Faraday Rotation (FR) in Support of the Solar Orbiter and Solar Probe Plus Missions
Mario Mark Bisi1, Alessandra S Giunta2, Elizabeth A Jensen3, Bernard V Jackson4, Richard Andrew Fallows5, Oyuki Chang6, Americo Gonzalez-Esparza7, Ernesto Aguilar-Rodriguez8, David Barnes2, Munetoshi Tokumaru9, Periasamy K Manoharan10, Dusan Odstrcil11,12, Hsiu-Shan Yu13 and David Wexler, MD, PhD14,15, (1)United Kingdom Research and Innovation - Science & Technology Facilities Council, Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom, (2)STFC Rutherford Appleton Laboratory, RAL Space, Harwell Campus, Didcot, United Kingdom, (3)Planetary Science Institute Tucson, Tucson, United States, (4)University of California, San Diego, Astronomy and Astrophysics, La Jolla, CA, United States, (5)ASTRON, The Netherlands Institute for Radio Astronomy, Dwingeloo, Netherlands, (6)Universidad Nacional Autonoma de Mexico, Posgrado en Ciencias de la Tierra, Mexico City, Mexico, (7)Universidad Nacional Autonoma de Mexico, LANCE, Instituto de Geofisica, Unidad Michoacan, Morelia, Mexico, (8)Universidad Nacional Autonoma de Mexico, Instituto de Geofisica, Unidad Michoacan, Morelia, Mexico, (9)Nagoya University, Institute for Space-Earth Environmental, Nagoya, Japan, (10)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States, (11)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (12)George Mason University, Fairfax, United States, (13)University of California San Diego, Center for Astrophysics and Space Science, La Jolla, CA, United States, (14)University of Southern Queensland, Toowoomba, Australia, (15)MIT Haystack Observatory, Westford, MA, United States
