Chihiro TAO websight        English

垰 千尋

Ecole Polytechnique, Laboratoire de Physique des Plasmas (LPP), 研究員
連絡先： chihiro.tao *at* lpp.polytechnique.fr

-----研究興味--------
木星土星超高層大気・電磁気圏物理学

主なテーマ
・木星磁気圏の太陽風応答
・木星超高層モデリングによるオーロラ形成と多圏間角運動量輸送
・木星・土星オーロラ発光モデル
・太陽風データ同化


-----研究関連資料--------
太陽風シミュレーションデータ ＠木星 ＠土星


-----論文--------
[18] O'Donoghue, J., T. S. Stallard, H. Melin, S. W. H. Cowley, S. V. Badman, L. Moore, S. Miller, C. Tao, K. H. Baines, and J. S. D. Blake, Conjugate observations of Saturn's northern and southern H3+ aurorae, Icarus, accepted.

[17] Kimura, T., L. Lamy, C. Tao, S. V. Badman, S. Kasahara, B. Cecconi, P. Zarka, A. Morioka, Y. Miyoshi, D. Maruno, Y. Kasaba, and M. Fujimoto (2013), Long-term modulations of Saturn's auroral radio emissions by the solar wind and seasonal variations controlled by the solar ultraviolet flux, J. Geophys. Res. Space Physics, 118, doi:10.1002/2013JA018833.

[16] Kita, H., H. Misawa, F. Tsuchiya, C. Tao, and A. Morioka (2013), Effect of solar UV/EUV heating on the intensity and spatial distribution of Jupiter's synchrotron radiation, J. Geophys. Res. Space Physics, 118, doi:10.1002/jgra.50568.

[15] Yoneda, M., F. Tsuchiya, H. Misawa, Bonfond B., Tao C., M. Kagitani and S. Okano (2013), Io's volcanism controls Jupiter's radio emissions, Geophys. Res. Lett. 40, doi:10.1002/grl.50095.

[14] Kasahara, S., E. A. Kronberg, T. Kimura, C. Tao, S. V. Badman, A. Masters, A. Retino, N. Krupp, and M. Fujimoto (2013), Asymmetric distribution of reconnection jet fronts in the Jovian nightside magnetosphere, J. Geophys. Res. Space Physics, 118, 375-384, doi:10.1029/2012JA018130.

[13] Badman, S. V., D. J. Andrews, S. W. H. Cowley, L. Lamy, G. Provan, C. Tao, S. Kasahara, T. Kimura, H. Melin, M. Fujimoto, T. Stallard, R. H. H. Brown, and K. H. H. Baines (2012), Rotational modulation and local time dependence of Saturn’s infrared H3+ auroral intensity, J. Geophys. Res., 117, A09228, doi:10.1029/2012JA017990.

[12] Tao, C., S. V. Badman, T. Uno, and M. Fujimoto (2012), On the feasibility of characterizing Jovian auroral electrons, via H3+ infrared line-emission analysis, Icarus, 221, 236-247.

[11] Tao, C., S. V. Badman, and M. Fujimoto (2012), Characteristic time scales of UV and IR auroral emissions at Jupiter and Saturn and their possible observable effects, ISPS proceeding paper, accepted.

[10] 垰 千尋, 藤本 正樹, 国際共同木星探査ワーキンググループ (2012), 探査機高緯度軌道からの木星オーロラ・プラズマ撮像サイエンス, 遊星人, 2012年3月号, 日本惑星科学会.

[9] 宇野 健, 坂野井 健, 垰 千尋, 笠羽 康正 (2012), 地上近赤外観測で捉える木星極域の熱圏大気, 遊星人, 2012年3月号, 日本惑星科学会.

[8] [8’] Badman, S. V., N. Achilleos, C. S. Arridge, K. H. Baines, R. H. Brown, E. J. Bunce, A. J. Coates, S. W. H. Cowley, M. K. Dougherty, M. Fujimoto, G. Hospodarsky, S. Kasahara, T. Kimura, H. Melin, D. G. Mitchell, T. Stallard, C. Tao (2012), Cassini observations of ion and electron beams at Saturn and their relationship to infrared auroral arcs, J. Geophys. Res., 117, A01211, doi:10.1029/2011JA017222.

[7] Kasahara, S., E. A. Kronberg, N. Krupp, T. Kimura, C. Tao, S. V. Badman, A. Retin`o, and M. Fujimoto (2011), Magnetic reconnection in the Jovian tail: X-line evolution and consequent plasma sheet structures, J. Geophys. Res., 116, A11219, doi:10.1029/2011JA016892.

[6] Badman, S. V., C. Tao, A. Grocott, S. Kasahara, H. Melin, R. H. Brown, K. H. Baines, M. Fujimoto, T. Stallard (2011), Cassini VIMS observations of latitudinal and hemispheric variations in Saturn’s infrared auroral intensity, Icarus, 216, 367-375.

[5] Tao, C., S. V. Badman, M. Fujimoto (2011), UV and IR auroral emission model for the outer planets: Jupiter and Saturn comparison, Icarus, 213, 581-592.

[4] Tao, C., H. Fujiwara, and Y. Kasaba (2010), Jovian magnetosphere-ionosphere current system characterized by diurnal variation of ionospheric conductance, Planet. Space Sci., 58, 351-364.

[3] Tao, C., H. Fujiwara, and Y. Kasaba (2009), Neutral wind control of the Jovian magnetosphere-ionosphere current system, J. Geophys. Res., 114, A08307, doi:10.1029/2008JA013966.

[2] Hiraki, Y., and C. Tao (2008), Parameterization of ionization rate by auroral electron precipitation in Jupiter, Ann. Geophys., 26, 77-86.

[1] Tao, C., R. Kataoka, H. Fukunishi, Y. Takahashi, and T. Yokoyama (2005), Magnetic field variations in the Jovian magnetotail induced by solar wind dynamic pressure enhancements, J. Geophys. Res., 110, A11208, doi:10.1029/2004JA010959.


-----国内外の学会・研究会発表 (2004-)--------
リスト

-----略歴--------

垰 千尋
たお ちひろ

博士(理学)

Ecole Polytechnique, Laboratoire de Physique des Plasmas (LPP), PostDoc researcher 2013/01-

宇宙航空研究開発機構 宇宙科学研究所 プロジェクト研究員, 2010/04-2012/12
JST/CREST 研究員, 2009/04-2010/03,
東北大学大学院理学研究科 地球物理学専攻 客員研究者, 2009/04-2010/03
日本学術振興会 特別研究員-DC2, 2007/04-2009/03
東北大学大学院理学研究科博士課程後期, 2006/04-2009/03
東北大学大学院理学研究科博士課程前期, 2004/04-2006/03
東北大学理学部宇宙地球物理学科, 2000/04-2004/03


最終更新日 2013/11/19