Zobrazeno 1 - 10
of 20
pro vyhledávání: '"位置分解能"'
Autor:
Nonoyama, Masayuki, Yamada, Hideaki, Haraguchi, Kentaro, Tamura, Keisuke, Ogasaka, Yasushi, Tawara, Yuzuru, Yamashita, Kojun
Publikováno v:
第4回宇宙科学シンポジウム = Proceedings of the 4th Space Science Symposium. :507-510
資料番号: AA0047899122
Autor:
Watanabe, Toshiaki, Watanabe, Takashi, Tobari, Hiroyuki, Hattori, Kunihiko, Ando, Akira, Inutake, Masaaki
Publikováno v:
宇宙輸送シンポジウム 平成15年度 = Proceedings of Space Transportation Symposium FY2003. :352-355
資料番号: AA0047118087
Autor:
Kodama, Shinsuke, Haruyama, Junichi, Otake, Makiko, Matsunaga, Tsuneo, Hirata, Naru, Nakamura, Ryosuke
Publikováno v:
第37回月・惑星シンポジウム = Proceedings of the 37th ISAS Lunar and Planetary Symposium. :179-182
The pre-flight calibration data of Lunar Imager/Spectrometer (LISM) onboard SELENE was derived in order to evaluate optical performance. The standard light directly calibrated by the blackbody was observed with the LISM flight model. The S/N ratios a
Publikováno v:
第37回月・惑星シンポジウム = Proceedings of the 37th ISAS Lunar and Planetary Symposium. :147-150
In order to monitor the mass loading on the Io plasma torus, ground-based Doppler-resolved imaging observation of [SII] 671.6 nm emission was carried out using an Imaging Fabry-Perot Interferometer (lambda/delta(lambda) approximately equal to 61,000)
Autor:
Okada, Tatsuaki, Shirai, Kei, Yamamoto, Yukio, Arai, Takehiko, Ogawa, Kazunori, Hosono, Kozue, Kato, Manabu
Publikováno v:
第37回月・惑星シンポジウム = Proceedings of the 37th ISAS Lunar and Planetary Symposium. :183-186
An X-ray fluorescence spectrometer, XRS, has been developed for the SELENE mission, a Japanese lunar polar orbiter that awaits its launch in 2006. The XRS will map major elemental composition of lunar surface with less than 20 km in spatial resolutio
Publikováno v:
第37回月・惑星シンポジウム = Proceedings of the 37th ISAS Lunar and Planetary Symposium. :119-122
Petrologic mapping of the Moon is performed with the use of Al-Mg and Fe-Mg petrologic techniques. Relative content of elements is estimated for end-member rock types (mare basalts, ferroan anorthosites, Mg-rich rocks). Perspectives of the method for
Autor:
Aoki, Shigeki, Kobayashi, Tadashi, Nishimura, Jun, Yamagami, Takamasa, Sato, Yoshihiro, Yuda, Toshinori, Kodama, Koichi, Niwa, Kimio, Hoshino, Kaoru, Nakamura, Mitsuhiro
Publikováno v:
大気球シンポジウム 平成15年度 = Balloon Symposium 2003. :145-148
資料番号: AA0046651038
Autor:
Saito, Masaharu, Takata, Toshiko, Chishima, Takuro, Matsushita, Masato, Ikeda, Yuji, Hirao, Naohisa, Iijima, Yoshimi
Publikováno v:
第37回月・惑星シンポジウム = Proceedings of the 37th ISAS Lunar and Planetary Symposium. :123-126
In order to understand mineral abundance of the lunar surface and resulting spectral analysis of the lunar surface, ground-based Lunar VIS/NIR Spectral Imager is developed. The spectral imager can acquire obtain three dimentional spectral and spatial
Autor:
Saito, Yasuyuki, Hikida, Hajime, Yokota, Yasuhiro, Shiraishi, Hiroaki, Tanaka, Satoshi, Mizutani, Hitoshi
Publikováno v:
第36回月・惑星シンポジウム = Proceedings of the 36th ISAS Lunar and Planetary Symposium. :157-160
The past studies showed that surface heat, flow of the Moon obtained by the Apollo missions, does not, properly represent the regional averages due to a heat-flow focusing effect of the megaregolith, however the past studies used unrealistic models,
Autor:
Kameno, Seiji, Wajima, Kiyoaki
Publikováno v:
平成14年度宇宙放射線シンポジウム:次期X線天文衛星NeXTは何を目指すか = Cosmic Radiation Symposium 2002: New Science to be Explored by the X-ray Astronomy Mission NeXT. :77-80
電波天文衛星「はるか」を使ったVSOPやその他の電波観測は、活動銀河核(AGN)のシンクロトロン放射を1ミリ秒を切る分解能で撮像することができる。この高空間分解能を活かして、ジェッ