Zobrazeno 1 - 10
of 26
pro vyhledávání: '"放射圧"'
Autor:
Yamakawa, Hiroshi
Publikováno v:
宇宙航空研究開発機構特別資料: 低推力・連続加速を用いた宇宙ミッションに関する研究会論文集 = JAXA Special Publication: Collection of Papers Presented at the Meeting on the Study of Space Missions Propelled by Low-Thrust and Sustained Acceleration. :33-38
Orbital dynamics of consecutive, low-thrust trajectories is overviewed. Focusing on the thrust direction constraints (e.g., transversal and radial thrust direction constraints), various trajectory design strategies of low-thrust missions are summariz
Publikováno v:
第7回宇宙科学シンポジウム = Proceedings of the 7th Space Science Symposium. :727-731
資料番号: AA0063354022
Autor:
Araya, Akito
Publikováno v:
VLBI技術による宇宙研究シンポジウム = Symposium on Space Research with VLBI Technology. :49-52
資料番号: AA0063348002
Publikováno v:
第39回月・惑星シンポジウム = Proceedings of the 39th ISAS Lunar and Planetary Symposium. :146-149
We investigate the sublimation effect on dust-deblis disks. We assume a constant dust production. When we consider migration of dust grains only due to Poynting-Robertson effect, the surface number density is constant for radial distance. The sublima
Autor:
Fujiwara, Daisuke, Watanabe, Seiichiro
Publikováno v:
第38回月・惑星シンポジウム = Proceedings of the 38th ISAS Lunar and Planetary Symposium. :124-127
We perform numerical simulations of the radial circulation of the dust in weak turbulent protoplanetary disks, taking the effect of radiation pressure of the central star and puffed-up inner rim of the disk into account. We confirm that the following
Publikováno v:
第38回月・惑星シンポジウム = Proceedings of the 38th ISAS Lunar and Planetary Symposium. :9-12
21P Giacobini Zinner (hereafter 21P/GZ) is known for the parent comet of the Draconids which made spectacular showers in 1933 and 1946. Hence 21P/GZ is likely to have a dense dust trail. We searched the faint scattered light of 21P/GZ on May 23, 2004
Autor:
Chun, Moo-Young, Kwon, Suk Minn, Ishiguro, Masateru, Sarugaku, Yuki, Miura, Naoya, Usui, Fumihiko, Ueno, Munetaka
Publikováno v:
第38回月・惑星シンポジウム = Proceedings of the 38th ISAS Lunar and Planetary Symposium. :1-4
Cometary dust trails are composed of large debris ejected from periodic comets. They were first detected in optical wavelength by our group using Kiso 1.05-m Schmidt. The sophisticated data reduction processes as well as the advanced instruments are
Publikováno v:
第15回アストロダイナミクスシンポジウム講演後刷り集 2005 = Proceedings of 15th Workshop on JAXA Astrodynamics and Flight Mechanics. :239-245
先ず、軌道上の太陽発電衛星のダイナミックスを解くために、数値シミュレータを開発している。シミュレータでは、系の構造柔軟性をバネで接続された多剛体により近似し、ニュート
Autor:
Saglam, Adem
Publikováno v:
第15回アストロダイナミクスシンポジウム講演後刷り集 2005 = Proceedings of 15th Workshop on JAXA Astrodynamics and Flight Mechanics. :232-238
To observe a celestial body far away with a good angular resolution, it is necessary to build telescopes with large diameters. Due to the atmospheric turbulence, increasing the diameter of the primary mirror above a certain limit does not improve the
Publikováno v:
平成16年度アストロダイナミクスシンポジウム:講演後刷り集 = ISAS proceedings of 14th Workshop on Astrodynamics and Flight Mechanics 2004: A Collection of Technical Papers. :61-66
編隊飛行する太陽発電衛星システム(FF-SSPS)は、静止軌道上にあって地球指向する発送電部と、太陽輻射圧を揚力として利用して赤道面から一定の距離に保たれつつ太陽指向する反射鏡に