日本地球惑星科学連合2025年大会

講演情報

[J] 口頭発表

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

2025年5月26日(月) 15:30 〜 17:00 展示場特設会場 (5) (幕張メッセ国際展示場 7・8ホール)

コンビーナ:江波 進一(国立大学法人筑波大学)、入江 仁士(千葉大学環境リモートセンシング研究センター)、石戸谷 重之(産業技術総合研究所)、中山 智喜(長崎大学 大学院水産・環境科学総合研究科)、座長:玄 大雄(中央大学)

16:15 〜 16:30

[AAS11-27] Source-Specific Light Absorptivity of Organic Aerosols: Insights From a Year-long Offline Study in Hyytiälä, Finland

*孫 銭哲1、周 瑞辰2、大畑 祥2、Shirota Chiaki3、Petäjä Tuukka4、Ahonen Lauri4、Kulmala Markku4持田 陸宏1,2 (1.名古屋大学大学院環境科学研究科、2.名古屋大学宇宙地球環境研究所、3.村田計測器サービス株式会社、4.ヘルシンキ大学大気地球システム研究所(INAR)/物理学)


キーワード:エアロゾル、光吸収、源解析、北方林

Various and complex chemical compositions were exhibited by organic aerosols (OAs) from different emission sources, and their light-absorbing properties and the contributions from different light-absorbing components remain inadequately characterized. In this study, the sources of OAs and their light absorption characteristics in Hyytiälä Forest Station were investigated for submicrometer particles collected on filters in the period from July 2021 to June 2022. OA extract solutions were prepared according to their solubility and polarity as high-polarity fraction (HP-WSOM), humic-like substances (HULIS), and water-insoluble organic matter (WISOM). The fractions were analyzed by the offline use of a high-resolution aerosol mass spectrometer (AMS), and a UV–visible spectrophotometer. Among the fractions, HP-WSOM on average had the highest O/C ratio (0.93±0.23), followed by HULIS (0.60±0.06), and WISOM (0.28±0.05). Two distinct source apportionment solutions were obtained from positive matrix factorization for the OA fractions. Both solutions resolved three common sources: fossil fuel OA, biogenic secondary OA (BSOA), and more-oxidized oxygenated OA (MO-OOA). The 4-factor solution further differentiated biomass burning OA (BBOA) into two subtypes: BBOA1 (characterized by CHN-family ions, indicative of fresh biomass combustion) and BBOA2 (marked by aromatic compounds, associated with aged biomass material/fossil fuel burning). Notably, mass absorption efficiency (MAE) for HP-WSOM, HULIS, and WISOM showed strong positive correlations (R= 0.64 – 0.73) with CHN-family, which were characteristic ions of BBOA-1. Multilinear regression analysis with non-negative constraints revealed distinct MAE values for different factors: BBOA1 demonstrated significantly higher light-absorbing capacity (MAE= 0.98 m²/g) compared to BBOA2 (MAE= 0.34 m²/g), and contributed 72.5% of total OA light absorption. This study suggested the applicability of AMS-derived CHN-family ions as a tracer for BBOA, and would provide the first field evidence for differentiating the contributions of fresh and aged biomass material burning aerosols to light absorption.