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Publikováno v:
第36回月・惑星シンポジウム = Proceedings of the 36th ISAS Lunar and Planetary Symposium. :262-265
Experimental studies of coalescence between MgO grains and SiO2 grains in smoke reveal the direct production of crystalline forsterite grains and amorphous Mg-bearing silicate owing to the difference of cooling velocity after the formation of Mg2SiO4