Zobrazeno 1 - 10 of 67 pro vyhledávání: '"木星"'
1
磁场与行星环境的演化 Evolution of the magnetic field and the planetary environment
行星的磁场会影响行星的环境演变,一颗具有较强磁场的行星,其磁场可以使这颗行星变成适宜生命的诞生的星球。然而磁场对行星具体产生作用的方式是什么?又是如何影响去行星环境的演变?
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::b02d833a928fcd7f800d33dde0e128b8
Zobrazit plný text záznamu
2
磁场与行星环境的演化 Evolution of the magnetic field and the planetary environment
Autor: 杨林
行星的磁场会影响行星的环境演变,一颗具有较强磁场的行星,其磁场可以使这颗行星变成适宜生命的诞生的星球。然而磁场对行星具体产生作用的方式是什么?又是如何影响去行星环境的演变?
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::b30249669399be400a5d47eea6271191
Zobrazit plný text záznamu
4
木星磁気圏探査ミッションのための木星系ツアー軌道設計
Autor: Tsuda, Yuichi
Publikováno v: 第17回アストロダイナミクスシンポジウム講演後刷り集 2007 = Proceedings of 17th Workshop on JAXA Astrodynamics and Flight Mechanics. :304-310
木星系ツアーのための軌道設計について考察する。木星磁気圏を探査するミッションを想定した場合、オービターは赤道面上の幅広い領域を通過することを要求される。木星周回軌道を
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::f351861ed4a11212ec721a8f672ff51a
http://id.nii.ac.jp/1696/00007481/
Zobrazit plný text záznamu
5
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/
Zobrazit plný text záznamu
6
Numerical modeling of moist convection in Jupiter's atmosphere: The dependency on the abundances of condensible volatiles
Autor: Sugiyama, Koichiro, Odaka, Masatsugu, Nakajima, Kensuke, Hayashi, Yoshiyuki
Publikováno v: 第40回月・惑星シンポジウム = Proceedings of the 40th ISAS Lunar and Planetary Symposium. :137-140
We develop a two-dimensional fluid dynamical model that incorporates condensation of H2O and NH3 and the production reaction of NH4SH. We run the model for a long simulation time in order to examine the structure of moist convection layer in Jupiter'
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::b5f2d34f148b7d59586532d604c1af2c
http://id.nii.ac.jp/1696/00020446/
Zobrazit plný text záznamu
7
木星探査における低弾道エアロキャプチャの可能性
Autor: Furukawa, Munetaka, Abe, Takashi
Publikováno v: 第16回アストロダイナミクスシンポジウム講演後刷り集 2006 = Proceedings of 16th Workshop on JAXA Astrodynamics and Flight Mechanics. :362-370
エアロキャプチャは、従来の化学推進による手段と比較して、軌道投入に要する推進剤を減らすことが可能であると知られている。 突入飛行経路角のウィンドウや空力加熱環境などの厳
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::55d48654c28232512d2155d8765cd85c
http://id.nii.ac.jp/1696/00007557/
Zobrazit plný text záznamu
9
Technology improvement in assessment of planetary entry environments and prediction of thermal protection system performance
Autor: Fujita, Kazuhisa, Matsuyama, Shingo, Suzuki, Toshiyuki, Matsukawa, Yutaka
Publikováno v: 宇宙航空研究開発機構特別資料: 平成18年度 宇宙航空研究開発機構 総合技術研究本部 宇宙科学研究本部 研究成果報告書 = JAXA Special Publication: Report on Research Achievements for FY2006 Institute of Space and Astronautical Science, Institute of Aerospace Technology, Japan Aerospace Exploration Agency. :103-106
Comprehensive researches on high-enthalpy flows and associated thermal protection technologies have been conducted in Aerodynamic Research Group, IAT, in cooperation with other research groups in JAXA. In this article, an over-view and the current st
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::5ba721af934d139484dcd4b7ba2ab46a
http://id.nii.ac.jp/1696/00006000/
Zobrazit plný text záznamu
10
Characteristics of short term variations of the Jovian synchrotron radiation at a frequency of 327 MHz
Autor: Nomura, Shiho, Misawa, Hiroaki, Tsuchiya, Fuminori, Morioka, Akira
Publikováno v: 第39回月・惑星シンポジウム = Proceedings of the 39th ISAS Lunar and Planetary Symposium. :33-36
The Jovian Synchrotron Radiation (JSR) is a radio wave emitted from the relativistic electrons in the Jovian radiation belt, which has information of dynamics of high-energy particles and electromagnetic disturbances in the Jovian inner magnetosphere
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::4d048b6823e26d20b87304eeb475b226
http://id.nii.ac.jp/1696/00020465/
Zobrazit plný text záznamu

Vyhledávací nástroje:

Upřesnit hledání

Omezení vyhledávání
Plný text Recenzováno Digitální knihovna AV ČR
Zdroje