日本地球惑星科学連合2021年大会

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-CG36] 衛星による地球環境観測

2021年6月3日(木) 17:15 〜 18:30 Ch.06

コンビーナ:沖 理子(宇宙航空研究開発機構)、本多 嘉明(千葉大学環境リモートセンシング研究センター)、高薮 縁(東京大学 大気海洋研究所)、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)

17:15 〜 18:30

[ACG36-P16] Wildfire watch using SWIR data from SGLI/GCOM-C

*栗原 幸雄1、村上 浩1 (1.宇宙航空研究開発機構 地球観測研究センター)

キーワード:森林火災、SGLI、しきさい

The Second-generation Global Imager (SGLI) is an optical sensor onboard the GCOM-C satellite. SGLI has eleven channels for visible to near-infrared wave range, six channels for short-wavelength to thermal infrared wave range, and two polarization channels for visible and near-infrared wavelength. The spatial resolution is switchable between 250 m and 1 km. In terms of watching wildfire, the spatial resolution of 250 m is an advantage of SGLI. Although lack of mid-infrared (MIR) channels is a disadvantage, SGLI has channels in a short-wavelength infrared (SWIR) range where data is sensitive to high temperatures.

We examined the SWIR data for its performance of watching wildfire. We introduced a threshold-based test for detecting hotspots and a single-channel method to estimate fire radiative power (FRP). The single-channel method followed Wooster et al. 2003. Preliminary results show good agreements with those retrieved from Himawari-8 data. Meanwhile, some of the SWIR data were saturated probably by some wildfire flaming in a wide area. That suggests the upper limit of the dynamic range of SWIR channels is too low for estimating FRP; this is likely to be originated from a mismatch between the high spatial resolution and the narrow dynamic range. However, SWIR can capture signs from wildfire behind the clouds and has detected hotspots that Himawari-8 could not, suggesting wildfire data from SGLI is worthy.