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Reiser, J. T.*; Neeway, J. J.*; Cooley, S. K.*; Parruzot, B.*; Heredia-Langner, A.*; Gin, S.*; Thomas, M.*; Smith, N. J.*; Icenhower, J. P.*; Stone-Weiss, N.*; et al.
International Journal of Applied Glass Science, 16(4), p.e16707_1 - e16707_16, 2025/10
被引用回数:0 パーセンタイル:0.00(Materials Science, Ceramics)A new technique, termed the stirred-reactor coupon analysis (SRCA) method, has been developed to measure the rate of glass dissolution in forward-rate conditions. Monolithic glass coupons are partially masked with an inert material before placement in a large volume of well-mixed solution with known chemistry and temperature for a predetermined duration. After the test, the mask is removed, and the difference in step height between the protected area and the exposed corroded portions of the sample coupon is measured to determine the extent of glass dissolution. The step height is converted to a rate measurement using the test duration and glass density. Test parameters such as sample surface preparation and test duration were evaluated to determine their effects on the measured rates. Additionally, results from an interlaboratory study (ILS) consisting of 12 laboratories from 11 different institutions are presented, where each laboratory performed 12 independent tests. When removing experimental outlier data, the 95% reproducibility limits for the SRCA method has no statistical difference with previously published standardized test methods used to determine the forward rate of glass dissolution. Overall, this paper describes steps necessary to perform the test method and provides the statistical calculations to evaluate test accuracy.
Barucci, M. A.*; Reess, J.-M.*; Bernardi, P.*; Doressoundiram, A.*; Fornasier, S.*; Le Du, M.*; 岩田 隆浩*; 中川 広務*; 中村 智樹*; Andr
, Y.*; et al.
Earth, Planets and Space (Internet), 73(1), p.211_1 - 211_28, 2021/12
被引用回数:35 パーセンタイル:87.51(Geosciences, Multidisciplinary)MMX赤外線分光計(MIRS)は、宇宙航空研究開発機構(JAXA)のMMXミッションに搭載されているイメージング分光計である。MIRSは他の4つのフランス研究所との協力、フランス国立宇宙研究センター(CNES)の協力と財政支援、およびJAXAと三菱電機(MELCO)との緊密な協力によりパリ天文台で開発されている。この装置はMMXの科学的目的を完全に達成するべく設計されている。MIRSはフォボスとダイモスの表面組成の分析およびサンプリングサイトの選択時に使用される組成診断スペクトル機能を含む近赤外線スペクトルマップ機能をリモートで提供する。MIRSはまた、火星の大気、特に雲,塵,水蒸気などの空間的時間的変化についても観測を行う予定である。