Physical properties of the solar corona derived from radio scintillation observations with the Akatsuki spacecraft
Physical properties of the solar corona derived from radio scintillation observations with the Akatsuki spacecraft
Shota Chiba1, Takeshi Imamura2, Munetoshi Tokumaru3, Daikou Shiota4, Takuma Matsumoto5, Hiroki Ando6, Hiroshi Takeuchi7, Yasuhiro Murata7, Atsushi Yamazaki8, Bernd Häusler9, Martin Paetzold10, Kazumasa Iwai3, Go Murakami11, Yoshizumi Miyoshi12, Sami Asmar13, Luciano Iess14, Paolo Cappuccio15, Ivan di Stefano16 and Antonio Genova17, (1)University of Tokyo, Bunkyo-ku, Japan, (2)The University of Tokyo, Graduate School of Frontier Science, Kashiwa, Chiba, Japan, (3)Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Japan, (4)NICT National Institute of Information and Communications Technology, Tokyo, Japan, (5)NAOJ National Astronomical Observatory of Japan, Tokyo, Japan, (6)ISAS/JAXA, 3-1-1 Yoshinodai/Sag, Japan, (7)JAXA Japan Aerospace Exploration Agency, Sagamihara, Japan, (8)ISAS/JAXA, Sagamihara, Kanagawa, Japan, (9)Bundeswehr University Munich, Institute of Space Technology and Space Applications, Munich, Germany, (10)Universitaet Koeln, Koeln, Germany, (11)ISAS-JAXA, Sagamihara, Japan, (12)Nagoya University, Institute for Space-Earth Environmental Research (ISEE), Nagoya, Japan, (13)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (14)Univ. La Sapienza, Roma, Italy, (15)Sapienza University of Rome, Department of Mechanical and Aerospace Engineering, Rome, Italy, (16)Sapienza University of Rome, Rome, Italy, (17)Massachusetts Institute of Technology, Cambridge, United States