2021
DOI: 10.3390/s21134313
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Optical Design of Imaging Spectrometer Based on Linear Variable Filter for Nighttime Light Remote Sensing

Abstract: Nighttime light remote sensing has unique advantages on reflecting human activities, and thus has been used in many fields including estimating population and GDP, analyzing light pollution and monitoring disasters and conflict. However, the existing nighttime light remote sensors have many limitations because they are subject to one or more shortcomings such as coarse spatial resolution, restricted swath width and lack of multi-spectral data. Therefore, we propose an optical system of imaging spectrometer bas… Show more

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Cited by 12 publications
(5 citation statements)
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“…The biggest impact of the dual-gratings on the image quality of the optical system should be the impact on the diffraction limit. The diffraction limit of an optical system is shown in Equation (11).…”
Section: The Effect Of Double-gratings On Mtfmentioning
confidence: 99%
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“…The biggest impact of the dual-gratings on the image quality of the optical system should be the impact on the diffraction limit. The diffraction limit of an optical system is shown in Equation (11).…”
Section: The Effect Of Double-gratings On Mtfmentioning
confidence: 99%
“…Typical imaging spectrometers include HSI from America, ESA-HRIS and PRISM from ESA, COIS from US Navy's NEMO Program, FTHSI from MightySat II CHRIS on the European PROBA small satellite, and HYPERION on EO-1 satellite of America [10]. Nighttime light remote sensors that can capture imageries with high spectral and spatial resolution in a wide waveband and swath width were also investigated in [11]. In recent years, the need for high-performance imaging spectrometers that span an application space from satellite imagery to food safety has never been higher.…”
Section: Introductionmentioning
confidence: 99%
“…An LVF is a mature thin-film dispersive element and has many applications in space [4,5]. The spectral properties of LVFs have been studied in previous studies.…”
Section: Introductionmentioning
confidence: 99%
“…In accordance with the requirements of the on-orbit polarization calibration method, the polarization response properties of each instrument channel, i.e., the normalized Mueller matrix elements, need to be calibrated in the laboratory. The polarization spectrum reactivity of space remote sensing instruments is a key parameter for calibrating instruments in laboratories, and the results have practical significance for assessing the instrument’s performance [ 20 , 21 , 22 , 23 ]. This paper introduces the laboratory calibration of the UV hyperspectral instrument’s polarization properties and implements error correction for the system’s radiation transmission link, providing high-precision ground polarization calibration information for on-orbit polarization calibration.…”
Section: Introductionmentioning
confidence: 99%