@inproceedings{oai:jaxa.repo.nii.ac.jp:00020567,
 author = {上野, 宗孝 and 石黒, 正晃 and 臼井, 文彦 and 矢野, 創 and 今村, 剛 and 中村, 正人 and 佐藤, 毅彦 and 木股, 雅章 and Ueno, Munetaka and Ishiguro, Masateru and Usui, Fumihiko and Yano, Hajime and Imamura, Takeshi and Nakamura, Masato and Sato, Takehiko and Kimata, Masafumi},
 book = {第38回月・惑星シンポジウム, Proceedings of the 38th ISAS Lunar and Planetary Symposium},
 month = {Mar},
 note = {Recent observations by space telescopes and large aperture telescopes on the ground show the exo-zodiacal disks around stars. The origin and evolution of the zodiacal dust are not yet understood well, since the interplanetary dust cannot stay long under the Poynting-Robertson drag and by mutual collisions of dusts themselves. To sustain the zodiacal dust cloud, it requires continuous supplies of the interplanetary dust particle. We present a new observing project using the cruising phase of PLANET-C/VCO (Venus Climate Orbiter) mission. The PLANET-C/VCO mission, which is a spacecraft cruising through the interplanetary space toward Venus, is a unique opportunity to observe the zodiacal light from the various viewing points and will give us the spatial distribution of the dust cloud along the heliocentric distance as well as the resonance structures., 資料番号: AA0063350052},
 pages = {192--195},
 publisher = {宇宙航空研究開発機構宇宙科学研究本部, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS)},
 title = {Observation of the zodiacal light during the cruising phase of PLANET-C/VCO mission},
 year = {2006}
}