에어로졸 광학깊이를 이용한 에어로졸 크기분포 추출 연구
Study of Retrieving the Aerosol Size Distribution from Aerosol Optical Depths
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초록
본 연구에서는 250 nm와 1100 nm 사이에 있는 10개의 파장에서의 에어로졸 광학 깊이를 이용하여 에어로졸의 크기분포를 역산하는 연구를 수행하였다. 10개의 파장은 주요 대기 가스의 흡수선과 밴드를 피한 파장을 찾아서 선택하였다. 태양의 스펙트 럼을 얻기 위해서 태양 추적시스템과 분광기를 구축하고 자체적으로 장치를 검정하였다. 본 장치를 이용해서 총 광학 깊이를 구하고 가스의 흡수나 공기의 산란을 제거하여 에어로졸의 광학 깊이를 구했다. 이정점 분포를 지닌 에어로졸 크기 분포를 역산 하는 알고리즘을 제안하였고, 장치를 통해서 구한 에어로졸의 광학 깊이를 이용하여 다양한 임의의 대기 조건에서 그 크기분포를 역산하고 비교하였다. 이를 통하여 본 연구에서 사용한 방법론과 장치들이 미지의 입자 크기 분포를 추출하는데 매우 유용할 것으로 판단하였다.
Abstract
In this study, aerosol size distributions were retrieved from aerosol optical depth measured over a range of 10 wavelengths from 250 to 1100 nm. The 10 wavelengths were selected where there is no absorption of atmospheric gases. To obtain the solar spectrum, a home-made solar tracking system was developed and calibrated. Using this solar tracking system, total optical depths (TODs) were extracted for the 10 wavelengths using the Langley plot method, and aerosol optical depths (AODs) were obtained after removing the effects of gas absorption and Rayleigh scattering from the TODs. The algorithm for retrieving aerosol size distributions was suggested by assuming a bimodal aerosol size distribution. Aerosol size distributions were retrieved and compared under various arbitrary atmospheric conditions. Finally, we found that our solar tracking spectrometer is useful for retrieving the aerosol size distribution, even though we have little information about the aerosol’s refractive index.
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