ATMOSPHERIC CORRECTION APPROACH FOR SABIA-MAR OCEAN COLOR MISSION

被引:0
作者
Tauro, Carolina [1 ]
Labanda, Martin [1 ]
Floreani, Raul [1 ]
Valvassori, Gaston [1 ]
Avila, Milagros [1 ]
Godoy, Facundo [1 ]
Tan, Jing [2 ]
Frouin, Robert [2 ]
机构
[1] Comis Nacl Act Espaciales CONAE, Buenos Aires, Argentina
[2] Scripps Inst Oceanog, La Jolla, CA USA
来源
IGARSS 2023 - 2023 IEEE INTERNATIONAL GEOSCIENCE AND REMOTE SENSING SYMPOSIUM | 2023年
关键词
SABIA-Mar; Ocean Color Remote Sensing; Atmospheric Correction; Multi-Angle Configuration;
D O I
10.1109/IGARSS52108.2023.10282700
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
The SABIA-Mar satellite mission, developed by CONAE, aims to provide valuable information and products for studying marine ecosystems, the carbon cycle, coastal dynamics, and marine habitats. The SABIA-Mar main cameras (measuring from visible to short wave infra-red) have a non-conventional design, since each spectral band has different viewing angles, which raises a challenge for the application of traditional atmospheric correction (AC) schemes. This work presents a preliminary analysis, based on simulated data sets, of uncertainties in the AC algorithm proposed for SABIA-Mar to retrieve water reflectance. This algorithm, a version of the standard AC scheme, was applied to SABIA-Mar angular and spectral characteristics, and the results compared to those obtained assuming the same viewing geometry for all the spectral bands. Performance is slightly degraded for the SABIA-Mar geometrical configuration, but the statistical results meet the goals of the SABIA-Mar mission and the requirements for ocean color applications.
引用
收藏
页码:3954 / 3957
页数:4
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