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Short-term earthquake prediction is considered to be an urgent subject for the countries likeJapan with high seismic activity. Because it is concluded about 10 years ago that the former andconventional seismic measurement of crustal movements is not

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::decb7ed4d9c60592d4772aa7dac9ffb6
http://id.nii.ac.jp/1438/00006883/

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Magnetic reconnection signature in Jupiter's H3(+) auroral activity

Autor: Connerney, Jack, Sato, Takehiko, Tokumaru, Munetoshi, Hayashi, Keiji

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

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::76567e9834850f972da8d9401d070e5c
http://id.nii.ac.jp/1696/00020448/

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Overshielding of The Convection Electric Field in The Ionosphere

Autor: Y., Ishikawa, K.K., Hashimoto, T., Kikuchi, T., Watanabe, M., Kunitake, K., Ohtaka, Physical Sciences, Graduate School of Science, Ibaraki University, School of Policy Management, Kibi International University, Solar-Terrestrial Environment Laboratory, Nagoya University, National Institute of Information and Communications Technology

Publikováno v: 吉備国際大学政策マネジメント学部研究紀要 = Journal of Kibi International University School of Policy Management. 3:31-41

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::09b1b36be80eacfc92a5d7ec3596c890
http://id.nii.ac.jp/1320/00000681/

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Investigations of plasma environment of Jupiter's polar upper ionosphere by spectrum analysis of auroral radio emissions

Autor: Misawa, Hiroaki, Morioka, Akira, Nozawa, Hiromasa, Tsuchiya, Fuminori

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

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::ccb6de16a323d5d5b32e7c12b8601178
http://id.nii.ac.jp/1696/00020463/

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