@inproceedings{oai:jaxa.repo.nii.ac.jp:00020524,
 author = {林, 満 and 中本, 泰史 and 木多, 紀子 and 橘, 省吾 and Hayashi, Mitsuru R. and Nakamoto, Taishi and Kita, Noriko T. and Tachibana, Shogo},
 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 = {Shock-wave heating model is one of the plausible models for chondrule formation, though the generation of shock waves has not been understood clearly. In this study, we have carried out MHD (MagnetoHydroDynamic) simulations of X-ray flares and subsequent expansion of magnetic bubbles and we examine whether the conditions of the shock waves inside of the solar nebula are suitable for chondrule formation. We found that shock waves of about 15 km/s with velocity could be generated at the upper region of the solar nebula at 3 AU from the central star. Such shock conditions at the upper region of the nebula at 3 AU seem to be appropriate for chondrule formation., 資料番号: AA0063350009},
 pages = {33--36},
 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 = {Shock-wave heating chondrule formation: MHD simulation of shockwave propagation inside of the disk},
 year = {2006}
}