日本地球惑星科学連合2022年大会

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セッション記号 A (大気水圏科学) » A-AS 大気科学・気象学・大気環境

[A-AS11] 大気化学

2022年5月27日(金) 13:45 〜 15:15 201A (幕張メッセ国際会議場)

コンビーナ:内田 里沙(一般財団法人 日本自動車研究所)、コンビーナ:坂本 陽介(京都大学大学院地球環境学堂)、岩本 洋子(広島大学大学院統合生命科学研究科)、コンビーナ:石戸谷 重之(産業技術総合研究所)、座長:松井 仁志(名古屋大学大学院環境学研究科)

14:00 〜 14:15

[AAS11-13] Contribution of chemical budget of δD-CH4 on δD-H2O in the equatorial lower stratosphere

*山田 崇貴1、齋藤 楓大1,2、奈良 誠大1佐藤 知紘1、Walker Kaley3、中野 幸夫2笠井 康子1 (1.情報通信研究機構、2.東京学芸大学、3.トロント大学)

Water vapor plays a key role in determining the radiative cooling effect in the upper atmosphere (UA). Methane is the most abundant hydrocarbon, and its amount is rising in UA due to anthropogenic emissions from the surface. The water vapor in UA is produced through the oxidation reaction of CH4 + OH → H2O + CH3. In general, the isotopic ratio is a strong tracer of the molecular history such as source, sink, and processes. We have confirmed how much the contribution of CH4 oxidation on H2O formation by global satellite observation of δD-CH4 and δD-H2O from space.
We used the version 4.0 data of Atmospheric Chemistry Experiment - Fourier Transform Spectrometer (ACE-FTS) (launched in 2003 and still in operation) onboard SciSat-1 developed by the Canadian government. The vertical resolution of the ACE-FTS solar occultation observation is 3 km, and observation wavenumber ranges 750 – 4400 cm-1 including H2O, HDO, CH4, and CH3D lines.
The scatter plot between δD-H2O and δD-CH4 showed a linear relationship by using the observed data at altitudes of 20 – 30 km and latitudes of 15oS – 15oN. The result of least-squares linear regression shows that the coefficient of determination is over 0.8 and δD-H2O increased linearly with the decrease of about 64% of δD-CH4. We will present the contribution of the chemical budget of δD-CH4 on δD-H2O in the lower stratosphere.