Japan Geoscience Union Meeting 2019

Presentation information

[J] Poster

M (Multidisciplinary and Interdisciplinary) » M-SD Space Development & Earth Observation from Space

[M-SD44] Future Missions of Satellite Earth Observation

Wed. May 29, 2019 5:15 PM - 6:30 PM Poster Hall (International Exhibition Hall8, Makuhari Messe)

convener:Yoshiaki HONDA(Center for Environmental Remote Sensing, Chiba University), Yukari Takayabu(Atmosphere and Ocean Research Institute, the University of Tokyo), Shinichi Sobue(Japan Aerospace Exploration Agency), Yuki Kaneko(Japan Aerospace Exploration Agency)

[MSD44-P07] Proposal of satellite for observing large point sources of carbon dioxide

*Hirofumi Ohyama1, Tsuneo Matsunaga1, Isamu Morino1, Yukio Yoshida1, Makoto Saito1 (1.National Institute for Environmental Studies)

Keywords:Satellite, Carbon Dioxide, Large Point Source

We propose an earth-observing satellite that aims to quantify amounts of atmospheric carbon dioxide (CO2) emitted from large point sources (LPSs) such as thermal power plants and steel plants, which account for approximately 40% of energy-related CO2 emissions in the world. In the Global Stocktake Process under the Paris Agreement, each country is required to report sources and sinks of greenhouse gases (inventory) with sufficient accuracy. However, there are large uncertainties in the CO2 and methane (CH4) emissions from the LPSs, especially for the developing countries. Space-borne observation could be useful for quantifying and verifying the emissions from the LPSs, given that it provides column abundances in and out a plume with high spatial resolution. With regard to the LPS observation of CH4, several satellites with a footprint size of less than 1 km2 are developed recently: GHGSat series (2016 and 2019, GHGSat Inc. in Canada), COOL (2020, Bluefield Technologies Inc. in the U.S.), and MethaneSAT (2021, Environmental Defense Fund in the U.S.). That kind of CO2 satellite is, however, not planed. Our proposed satellite has an ability of measuring back-scattered solar spectra in the near-infrared region with a footprint size of less than 1 km x 1 km (if feasible, hundreds of meters by hundreds of meters) using an imaging grating spectrometer. Additionally, to increase the signal to noise ratio of the spectrum, the satellite is dedicated to a target observation mode that observe an area of ~50 km x ~50 km including the LPSs more than 2 min continuously by using a pointing mechanism as adopted for the Greenhouse gases Observing SATellite (GOSAT) series.