@inproceedings{oai:jaxa.repo.nii.ac.jp:00014683,
 author = {鈴木, 宏二郎 and Suzuki, Kojiro},
 book = {宇宙航行の力学シンポジウム　平成15年度, Symposium on Flight Mechanics and Astrodynamics 2003},
 month = {May},
 note = {When a solar probe penetrates into the solar corona for the in-situ observation of the solar wind, the temperature of its heat shield becomes extremely high and the sublimation of the surface material occurs. In the present study, both the near field and the far field analyses on the behavior of the sublimation gas injected from the C/C wall are made by the DSMC method. The former clarifies the number density distribution of the sublimation gas around the probe. The latter is made to simulate the interaction between the solar wind and the sublimation gas cloud. When the total sublimation rate becomes high at close approach to the sun, the length scale of the interaction phenomena becomes in the order of kilometers and the properties of the solar wind are highly disturbed by the presence of the probe itself., 資料番号: AA0047120038},
 pages = {147--150},
 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 = {ソーラープローブ熱シールドからの昇華ガスと太陽風の干渉に関する数値解析},
 year = {2004}
}