Abstract

The need to monitor specific areas for different applications requires high spatial and temporal resolution. This need has led to the proliferation of ad hoc systems on board nanosatellites, drones, etc. These systems require low cost, low power consumption, and low weight. The work we present follows this trend. Specifically, this article evaluates a method to determine the cloud map from the images provided by a simple bi-spectral infrared camera within the framework of JEM-EUSO (The Joint Experiment Missions-Extrem Universe Space Observatory). This program involves different experiments whose aim is determining properties of Ultra-High Energy Cosmic Ray (UHECR) via the detection of atmospheric fluorescence light. Since some of those projects use UV instruments on board space platforms, they require knowledge of the cloudiness state in the FoV of the instrument. For that reason, some systems will include an infrared (IR) camera. This study presents a test to generate a binary cloudiness mask (CM) over the ocean, employing bi-spectral IR data. The database is created from Moderate-Resolution Imaging Spectroradiometer (MODIS) data (bands 31 and 32). The CM is based on a split-window algorithm. It uses an estimation of the brightness temperature calculated from a statistical study of an IR images database along with an ancillary sea surface temperature. This statistical procedure to obtain the estimate of the brightness temperature is one of the novel contributions of this work. The difference between the measured and estimation of the brightness temperature determines whether a pixel is cover or clear. That classification requires defining several thresholds which depend on the scenarios. The procedure for determining those thresholds is also novel. Then, the results of the algorithm are compared with the MODIS CM. The agreement is above 90%. The performance of the proposed CM is similar to that of other studies. The validation also shows that cloud edges concentrate the vast majority of discrepancies with the MODIS CM. The relatively high accuracy of the algorithm is a relevant result for the JEM-EUSO program. Further work will combine the proposed algorithm with complementary studies in the framework of JEM-EUSO to reinforce the CM above the cloud edges.

Highlights

  • The detection of clouds with airborne instruments is critical when studying the meteorology and climate of the Earth

  • The main idea of the methodology we propose is to establish a relationship between the BT11, the Brightness Temperature Difference (BTD) between BT11 and BT12, and the ancillary SST using a set of real images in BT11 and BT12 bands

  • The comparison with the Pure Cloud Mask (PCM) ground truth, which evaluates the performance of the Split-Window Cloudiness Mask (SWCM) to classify clear and cloudy pixels, gives more satisfactory skill scores than the comparison with the Reference Cloud Mask (RCM) ground truth, which better reflect the overall skill of the SWCM including mixed pixels

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Summary

Introduction

The detection of clouds with airborne instruments is critical when studying the meteorology and climate of the Earth. There are other applications where auxiliary systems for cloud detection and characterization are needed, which is the case that concerns us. Thermography is one of the main techniques for measuring the temperature of things remotely. It is based on InfraRed (IR) cameras to characterize the relationship between the object temperature and the IR energy it emits. The first applications of IR cameras were military (World War II), their use spread to many fields since the 1960s. The direct application of IR cameras to some applications did not obtain the expected results

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