TY - JOUR
PY - 2022//
TI - Comparing geostationary and polar-orbiting satellite sensor estimates of Fire Radiative Power (FRP) during the Black Summer Fires (2019-2020) in south-eastern Australia
JO - International journal of wildland fire
A1 - Chatzopoulos-Vouzoglanis, Konstantinos
A1 - Reinke, Karin J.
A1 - Soto-Berelov, Mariela
A1 - Engel, Chermelle
A1 - Jones, Simon D.
A1 - Chatzopoulos-Vouzoglanis, Konstantinos
A1 - Reinke, Karin J.
A1 - Soto-Berelov, Mariela
A1 - Engel, Chermelle
A1 - Jones, Simon D.
SP - 572
EP - 585
VL - 31
IS - 6
N2 - Background We compared estimates of Fire Radiative Power (FRP) from sensors onboard geostationary Himawari-8 (BRIGHT_AHI) and polar-orbiting TERRA/AQUA (MOD14/MYD14) satellites during the 2019/2020 Black Summer Fires in South-Eastern Australia.Aim/methods Analysis was performed on a pixel, bioregion, and wildfire event basis to assess the utility of the new BRIGHT_AHI FRP product.Key results Results show a high agreement between the products (r = 0.74, P < 0.01) on a pixel level, with BRIGHT_AHI generally underestimating FRP compared to MOD14/MYD14. Regional spatiotemporal trends were captured in more detail by BRIGHT_AHI due to its higher temporal resolution, with MOD14/MYD14 systematically underestimating the total and sub-diurnal FRP values. Nevertheless, both datasets captured similar fire ignition and spread patterns for the study region. On the event level, the correlation between the datasets was moderate (r = 0.49, r = 0.67), when considering different temporal constraints for hotspot matching.
CONCLUSIONS The results of this study indicate that BRIGHT_AHI approximates the well-established MOD14/MYD14 product during concurrent observations, while revealing additional temporal information for FRP trends.Implications This gives confidence in the reliability of BRIGHT_AHI FRP estimates, opening the way for a denser observation record (10-min intervals) that will provide new opportunities for fire activity reporting, some of which are presented here.
Language: en
LA - en SN - 1049-8001 UR - http://dx.doi.org/10.1071/WF21144 ID - ref1 ER -