摘要
CO 2 ice has a phase transition at 30 K when its structure changes from amorphous to crystalline. Using reflection absorption infrared spectroscopy, berg et al. observed that the photodesorption yield of CO 2 ice deposited at 60 K and irradiated at 18 K is 40% lower than that of CO 2 ice deposited and irradiated at 18 K. In this work, CO 2 ices were deposited at 16-60 K and UV-irradiated at 16 K to rule out the temperature effect and figure out the relationship between photodesorption yield and ice structure. IR spectroscopy is a common method used for measurement of the photodesorption yield in ices. We found that undetectable C atoms produced in irradiated CO 2 ice can account for 33% of the amount of depleted CO 2 molecules in the ice. A quantitative calibration of QMS was therefore performed to convert the measured ion current into photodesorption yield. During various irradiation periods, the dominant photodesorbing species were CO, O 2 , and CO 2 , and their photodesorption yields in CO 2 ices deposited at different temperature configurations were almost the same, indicating that ice morphology has no effect on the photodesorption yield of CO 2 ice. In addition, we found that the lower desorption yield reported by Martín-Doménech et al. is due to a linear relationship between the photodesorption yield and the combination of the energy distribution of the Microwave-Discharge Hydrogen-flow Lamp and UV absorption cross section of ices.
原文 | ???core.languages.en_GB??? |
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文章編號 | 35 |
期刊 | Astrophysical Journal |
卷 | 874 |
發行號 | 1 |
DOIs | |
出版狀態 | 已出版 - 20 3月 2019 |