文献
J-GLOBAL ID:201902233016618381
整理番号:19A1463390
惑星規模の波と平均循環による金星雲頂におけるY特徴の形成:VenusエクスプレスVMC画像の解析【JST・京大機械翻訳】
Formation of the Y Feature at the Venusian Cloud Top by Planetary-Scale Waves and the Mean Circulation: Analysis of Venus Express VMC Images
著者 (9件):
Nara Y.
(Department of Complexity Science and Engineering, Graduate School of Frontier Sciences, The University of Tokyo, Kashiwa, Chiba, Japan)
,
Imamura T.
(Department of Complexity Science and Engineering, Graduate School of Frontier Sciences, The University of Tokyo, Kashiwa, Chiba, Japan)
,
Murakami S.
(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Kanagawa, Japan)
,
Kouyama T.
(National Institute of Advanced Industrial Science and Technology, Koto-ku, Tokyo, Japan)
,
Ogohara K.
(Department of Electronic System Engineering, School of Engineering, The University of Shiga Prefecture, Hikone, Shiga, Japan)
,
Yamada M.
(Planetary Exploration Research Center, Chiba Institute of Technology, Narashino, Chiba, Japan)
,
Takagi M.
(Faculty of Science, Kyoto Sangyo University, Kyoto, Japan)
,
Kashimura H.
(Center for Planetary Science/Department of Planetology, Graduate School of Science, Kobe University, Kobe, Hyogo, Japan)
,
Sato N.
(Natural Science Division, Tokyo Gakugei University, Koganei, Tokyo, Japan)
資料名:
Journal of Geophysical Research: Planets
(Journal of Geophysical Research: Planets)
巻:
124
号:
5
ページ:
1143-1156
発行年:
2019年
JST資料番号:
W2387A
ISSN:
2169-9097
CODEN:
JGREA2
資料種別:
逐次刊行物 (A)
記事区分:
原著論文
発行国:
アメリカ合衆国 (USA)
言語:
英語 (EN)