Gabriele Meoni, Roberto Del Prete, Lucia Ancos-Villa, Enrique Albalate-Prieto, David Rijlaarsdam, Jose Luis Espinosa-Aranda, Nicolas Longépé, Maria Daniela Graziano, Alfredo Renga
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引用次数: 0
摘要
如今,机器学习(ML)在地球观测(EO)卫星上的使用已经被研究用于依赖于多光谱和高光谱成像的大量应用。传统上,这些研究严重依赖于高端数据产品,受到广泛的预处理链的影响,这些预处理链是为在地面上执行而设计的。然而,在EO卫星上复制这样的算法面临着巨大的挑战,因为它们的计算强度和需要额外的元数据,而这些元数据通常在卫星上不可用。正因为如此,目前探索机载机器学习模型的任务实现了简化但仍然复杂的处理链,模仿了地面上的处理链。尽管取得了这些进步,但机器学习模型直接处理原始卫星数据的潜力在很大程度上仍未得到探索。为了填补这一空白,本文研究了将ML模型直接应用于Sentinel-2原始数据进行热热点分类的可行性。这种方法极大地限制了处理步骤的简单和轻量级算法,以实现低功耗数据的实时处理。为此,我们提出了一个端到端(E2E)管道来创建Sentinel-2原始颗粒的二元分类图,其中每个点都表明在2.5公里的平方区域内不存在热异常。为此,采用轻量化粗空间配准方法对3个不同波段进行配准,并用effentnet -lite0模型对不同波段进行分类。经过训练的模型在5个种子上的平均马修相关系数(MCC)得分为0.854,在THRawS数据集裁剪图像的地理三方数据集上的最大MCC得分为0.90。提出的E2E管道能够在1.8秒内处理Sentinel-2颗粒,在Raspberry PI 4和CogniSat-XE2板的组合上,峰值功率为6.4 W,具有实时性。
E2E: Onboard satellite real-time classification of thermal hotspots events on optical raw data
Nowadays, the use of Machine Learning (ML) onboard Earth Observation (EO) satellites has been investigated for a plethora of applications relying on multispectral and hyperspectral imaging. Traditionally, these studies have heavily relied on high-end data products, subjected to extensive pre-processing chains natively designed to be executed on the ground. However, replicating such algorithms onboard EO satellites poses significant challenges due to their computational intensity and need for additional metadata, which are typically unavailable on board. Because of that, current missions exploring onboard ML models implement simplified but still complex processing chains that imitate their on-ground counterparts. Despite these advancements, the potential of ML models to process raw satellite data directly remains largely unexplored. To fill this gap, this paper investigates the feasibility of applying ML models directly to Sentinel-2 raw data to perform thermal hotspot classification. This approach significantly limits the processing steps to simple and lightweight algorithms to achieve real-time processing of data with low power consumption. To this aim, we present an end-to-end (E2E) pipeline to create a binary classification map of Sentinel-2 raw granules, where each point suggests the absence/presence of a thermal anomaly in a square area of 2.5 km. To this aim, lightweight coarse spatial registration is applied to register three different bands, and an EfficientNet-lite0 model is used to perform the classification of the various bands. The trained models achieve an average Matthew’s correlation coefficient (MCC) score of 0.854 (on 5 seeds) and a maximum MCC of 0.90 on a geographically tripartite dataset of cropped images from the THRawS dataset. The proposed E2E pipeline is capable of processing a Sentinel-2 granule in 1.8 s and within 6.4 W peak power on a combination of Raspberry PI 4 and CogniSat-XE2 board, demonstrating real-time performance.
期刊介绍:
Astrodynamics is a peer-reviewed international journal that is co-published by Tsinghua University Press and Springer. The high-quality peer-reviewed articles of original research, comprehensive review, mission accomplishments, and technical comments in all fields of astrodynamics will be given priorities for publication. In addition, related research in astronomy and astrophysics that takes advantages of the analytical and computational methods of astrodynamics is also welcome. Astrodynamics would like to invite all of the astrodynamics specialists to submit their research articles to this new journal. Currently, the scope of the journal includes, but is not limited to:Fundamental orbital dynamicsSpacecraft trajectory optimization and space mission designOrbit determination and prediction, autonomous orbital navigationSpacecraft attitude determination, control, and dynamicsGuidance and control of spacecraft and space robotsSpacecraft constellation design and formation flyingModelling, analysis, and optimization of innovative space systemsNovel concepts for space engineering and interdisciplinary applicationsThe effort of the Editorial Board will be ensuring the journal to publish novel researches that advance the field, and will provide authors with a productive, fair, and timely review experience. It is our sincere hope that all researchers in the field of astrodynamics will eagerly access this journal, Astrodynamics, as either authors or readers, making it an illustrious journal that will shape our future space explorations and discoveries.