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首页> 外文期刊>Applied Surface Science >Identification Of Silicate And Carbonaceous Presolar Grains By Sims In The Type-3 Enstatite Chondrite Alha81189
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Identification Of Silicate And Carbonaceous Presolar Grains By Sims In The Type-3 Enstatite Chondrite Alha81189

机译:用Sims鉴定3型顽辉陨石Alha81189中的硅酸盐和碳质前太阳粒

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An isotope ratio imaging technique using the HokuDai isotope microscope system has been applied to in situ survey for presolar grains in the type-3 enstatite chondrite ALH A81189. Rastered and static ion beam were used for primary beam. Lateral resolution of the isotope image was achieved to be 0.4 μm for static ion beam mode and to be 0.6 μm for rastered ion beam mode. As a result, the abundances of presolar grains are 150-200% larger under the static ion beam mode than under the rastered ion beam mode. Development of image processing introducing isotopography of ~(32)S~-, ~(24)Mg~(16)O~- and ~(56)Fe~- succeeded to increase efficiency of presolar grain characterization. Using the static ion beam and introducing appropriate isotopography were very useful methods of in situ characterization of presolar grains in meteorites.
机译:使用HokuDai同位素显微镜系统的同位素比率成像技术已被用于就地调查3型顽辉石球粒陨石ALH A81189中的太阳前晶粒。光栅离子束和静态离子束用于主束。同位素图像的横向分辨率在静态离子束模式下达到0.4μm,在光栅离子束模式下达到0.6μm。结果,在静态离子束模式下,比在光栅离子束模式下,前太阳晶粒的丰度大了150-200%。引入〜(32)S〜-,〜(24)Mg〜(16)O〜-和〜(56)Fe〜-等值形貌的图像处理技术的发展成功地提高了太阳前晶粒表征的效率。使用静电离子束并引入适当的同位素,是对陨石中太阳前晶粒进行原位表征的非常有用的方法。

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