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1. H. Miura, T. Nakamoto, and M. Doi, Shock-Wave Heating Model for Chondrule Formation: Formation of Prolate Chondrules, Proceedings of the 39th ISAS Lunar and Planetary Symposium, 13-16, 2006
2. H. Miura and T. Nakamoto, Thermal history of chondrules during shock-wave heating, Antarctic Meteorite Research 18, 239-252, 2005
3. H. Miura and T. Nakamoto, Shock-Wave Heating Model for Chondrule Formation: Dynamics of Molten Droplet Exposed to Rarefied Gas Flow, Proceedings of the 38th ISAS Lunar and Planetary Symposium, 25-28, 2005
4. H. Miura and T. Nakamoto, Shock-Wave Heating Model for Chondrule Formation: Chondrule Formation in a Less-Dusty Environment, Proceedings of the 37th ISAS Lunar and Planetary Symposium (Edited by H. Mizutani and M. Kato), pp.41-44, 2004
5. H. Miura and T. Nakamoto, Crystallization of Silicates in Circumstellar Environments by Shock Waves, Proceedings of The 23th Grain Formation Workshop, 113-118, 2004
6. H. Miura, T. Nakamoto, and H. Susa, Chondrule Radius and Evaporate Fraction in Viewpoint of Shock-Wave Heating Model, Geochimica et Cosmochimica Acta 67, 18S, A295, 2003
7. H. Miura, T. Nakamoto, and H. Susa, A Shock-Wave Heating Model for Chondrule Formation: Peak Temperature of Precursor Particles and High Ambient Gas Pressure, IAU 8th Asian-Pacific Regional Meeting, ASP Conference Series 289, 169-170, 2003
8. H. Miura and T. Nakamoto, Explanation for Minimum Size of Chondrules by Shock-Wave Heating Model, Proceedings of the 36th ISAS Lunar and Planetary Symposium, 41-44, 2003
9. H. Miura, T. Nakamoto, and H. Susa, Effect of Evaporation for Chondrule Formation by Shock Heating, Proceedings of the 34th ISAS Lunar and Planetary Symposium, pp. 111-114, 2001

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