JpGU-AGU Joint Meeting 2020

講演情報

[E] ポスター発表

セッション記号 A (大気水圏科学) » A-CG 大気海洋・環境科学複合領域・一般

[A-CG49] Greenhouse Gas Monitoring from Space: Current Capabilities, Challenges, and Future Needs

コンビーナ:kurosu thomas p(Jet Propulsion Laboratory, California Institute of Technology)、Annmarie Eldering(Jet Propulsion Laboratory)、久世 暁彦(宇宙航空研究開発機構)、松永 恒雄(国立環境研究所地球環境研究センター/衛星観測センター)

[ACG49-P04] Global and local flux estimation of carbon dioxide and methane by GOSAT satellites

*久世 暁彦1Kikuchi Nobuhiro1Suto Hiroshi1Shiomi Kei1Kataoka Fumie2 (1.Japan Aerospace Exploration Agency、2.Remote Sensing Technology Center of Japan)

キーワード:GOSAT、greenhouse gases、flux、carbon dioxide、methane

GOSAT and GOSAT-2 have provided long-term radiance spectral data using Fourier transform spectrometer technology since 2009 and 2018, respectively. With the advantage of FTS multiplexing, they can simultaneously measure carbon dioxide (CO2) and methane (CH4) absorption bands of reflected solar light with two linear polarizations and thermal emission. Radiance spectra with two polarizations can distinguish between less-polarized reflections from the Earth’s surface and highly polarized scattering by aerosols and thin clouds. The infrared band can add information to vertical profiles. By combining all these spectra data, partial column densities of the upper (4-12 km) and lower (0–4 km) troposphere can be retrieved, even under thick aerosol regions such as Africa, India, and South Africa. Two-layer vertical information enhances measurements of near-surface emission and uptake and reduces errors in transportation, therefore improving global flux estimation. With two-axis pointing systems, they can target large point sources and mega cities and have enhanced measurements of CO2 and CH4. However, local flux estimates by GOSAT may be problematic because of too large a footprint, a lack of proper upwind reference observations, and insufficient wind information. To contribute to the global stocktake of the Paris Agreement, we need a system to observe and estimate local flux from individual source sectors. We will present the status of flux estimation and discuss how to reduce such uncertainties.