Abstract

The high-precision characterization of the intra-pixel sensitivity (IPS) for infrared focal plane array (FPA) photodetector is of great significance to high-precision photometry and astrometry in astronomy, as well as target tracking in under-sampled remote sensing images. The discrete sub-pixel response (DSPR) model and fill factor model have been used for IPS characterization in some studies. However, these models are incomplete and lack the description of physical process of charge diffusion and capacitance coupling, leading to the inaccuracy of IPS characterization. In this paper, we propose an improved IPS characterization method based on the diffusion and coupling physical (DCP) model for infrared FPA photodetector, which considering the processes of generation and collection of the charge, can improve the accuracy of IPS characterization. The IPS model can be obtained by convolving the ideal rectangular response function with the charge diffusion function and the capacitive coupling function. Then, the IPS model is convolved with the beam spot profile to obtain the beam spot scanning response model. Finally, we calculate the parameters of IPS by fitting the beam spot scanning response map with the proposed DCP model based on the Trust-Region-Reflective algorithm. Simulated results show that when using a 3 μm beam spot to scan, the error of IPS characterization based on DCP model is 0.63%, which is better than that of DSPR model’s 3.70%. Experimental results show that the fitting error of the beam spot scan response model based on DCP model is 4.29%, which is better than that of DSPR model’s 8.31%.

Highlights

  • Infrared focal plane array (FPA) photodetector is widely used in astronomical observation and remote sensing for point target tracking [1,2]

  • Some evaluation criteria are determined to verify the performance of the improved model for the intra-pixel sensitivity (IPS) characterization of the infrared FPA photodetector

  • As the true value of the IPS cannot be determined for the experimental test, the error of fitting for experimental beam spot scanning response map with the model in Equation (8) is used to evaluate the performance of the model

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Summary

Introduction

Infrared FPA photodetector is widely used in astronomical observation and remote sensing for point target tracking [1,2]. The non-uniformity of the IPS of the infrared FPA photodetector can be ignored when the optical PSF is oversampled. When the image is under-sampled, the non-uniformity of IPS has a significant effect on highprecision photometry and astrometry in astronomy as well as point target tracking in remote sensing [3,4,5]. The experimental measurement methods of IPS mainly include the interference pattern method based on frequency domain and beam spot scanning method [6]. Fourier transform is an effective method in the frequency domain [7,8]. The optical system of this method is very complex; the continuously self-imaging grating (CSIG)

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