[P-PS01] Outer Solar System Exploration Today, and Tomorrow

[PPS01-P12] Titan's Ionospheric Density Structure Derived by Polarized Saturnian Radio Occultations during Cassini's Titan 15 Flyby

Rikuto Yasuda¹, *Hiroaki Misawa¹, Baptiste Cecconi², Corentin K. Louis², Tomoki Kimura³, Takeru Kato¹, Yasumasa Kasaba¹, Thomas Gautier^4,2, Lucas Grosset², Shotaro Sakai⁵, Fuminori Tsuchiya¹ (1. Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University, 2. LIRA, Observatoire de Paris, 3. Department of Physics, Faculty of Science, Tokyo University of Science, 4. LATMOS/IPSL, UVSQ Universite Paris-Saclay, Sorbonne Universite, CNRS, 5. Faculty of Environment and Information Studies, Keio University)

Keywords:Saturn, Titan, radio occultation method, ionosphere, icy moon