@inproceedings{oai:jaxa.repo.nii.ac.jp:00007299, author = {川勝, 康弘 and Campagnola, Stefano and Kawakatsu, Yasuhiro}, book = {アストロダイナミクスシンポジウム講演後刷り集, The 20th Workshop on JAXA Astrodynamics and Flight Mechanics}, month = {Mar}, note = {第20回アストロダイナミクスシンポジウム (2010年7月26-27日. 宇宙航空研究開発機構宇宙科学研究所), 相模原市, 神奈川県, The 20th Workshop on JAXA Astrodynamics and Flight Mechanics 2010 (July 26-27, 2010. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)), Sagamihara, Kanagawa Japan, This paper study the 3D resonant hopping, which is a sequence of gravity assists at one moon connecting resonant orbits. The orbits are not necessarily coplanar, and the spacecraft can change its orbital elements within a wide range using gravity assists. The technique is especially useful for missions targeting high inclinations. However the solution space grows geometrically with the number of gravity assists, and its full exploration during preliminary design is challenging. In this paper we study the problem in general and derive some useful analytical formula and the 3D-Tisserand graph, which is an extension of the famed Tisserand graph. We use the formula in a fast branch& bound algorithm, with which we compute thousands of solution for the Jupiter Magnetosheric Orbiter, JAXA's planned mission to explore the Jovian magnetosphere and the plasma torus from high latitudes., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA0065115052}, pages = {318--325}, publisher = {宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS), Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)}, title = {Pumping the inclination on the Jupiter equator for the Jupiter Magnetospheric Orbiter}, volume = {20}, year = {2011} }