Zobrazeno 1 - 5
of 5
pro vyhledávání: '"惑星電離圏"'
Publikováno v:
第40回月・惑星シンポジウム = Proceedings of the 40th ISAS Lunar and Planetary Symposium. :147-150
We have compared time history of integrated flux of Jupiter's H3(+) aurora, acquired in 1998-2000, with the sola-wind database. The solar wind at Jupiter is simulated based on the MHD (MagnetoHydroDynamic) tomography analysis of InterPlanetary Scinti
Publikováno v:
第39回月・惑星シンポジウム = Proceedings of the 39th ISAS Lunar and Planetary Symposium. :25-28
For the purpose of confirming the plasma condition of the topside ionosphere, we have investigated spectra of Jupiter's radio emissions observed with the Cassini spacecraft to derive the Faraday rotation for the period of Cassini's Jupiter swing-by a
Autor:
Terada, Naoki, Martian Aeronomy Group
Publikováno v:
第39回月・惑星シンポジウム = Proceedings of the 39th ISAS Lunar and Planetary Symposium. :132-135
資料番号: AA0063505034
Autor:
Takahashi, Yukihiro, Sakanoi, Takeshi, Yamazaki, Atsushi, Yoshida, Jun, Yoshida, Kazuya, Nakanishi, Hiroki, Shoji, Yasuhiro, Kawasaki, Kohei, Taguchi, Makoto
Publikováno v:
第6回宇宙科学シンポジウム = Proceedings of the 6th Space Science Symposium. :407-450
資料番号: AA0063353044
Autor:
Sakanoi, Takeshi, Takahashi, Yukihiro, Yoshida, Kazuya, Taguchi, Makoto, Yamazaki, Atsushi, Yoshida, Jun, Nakanishi, Hiroki, Shoji, Yasuhiro, Kawasaki, Kohei
Publikováno v:
第5回宇宙科学シンポジウム = Proceedings of the 5th Space Science Symposium. :392-395
惑星観測は、これまで探査機による直接探査と地上望遠鏡による遠隔計測を主な手段としてきたが、どちらも一長一短がある。惑星の大気・プラズマ現象の解明のためには、連続的な時