The CSIM system incorporates a fused silica triangular prism that disperses the incoming light. The CSIM spectrometer is utilized for long-term measurements of solar spectral irradiance (SSI) to understand how solar variability affects Earth’s climate. On the other hand, the PRISMA instrument uses three prisms to achieve VNIR and SWIR channels with a spectral range of 400–1010 nm (66 bands) and 920–2505 nm (174 bands), respectively.
The APEX instrument consists of VNIR (Visible-Near-Infrared) and SWIR (Short-Wave-Infrared) channels, realized by CaF 2/ZnS and CaF 2/sapphire prisms, respectively. The APEX and PRISMA spectrometers are employed in remote sensing applications for soil, water, and atmosphere. VI, we provide concluding remarks and outline future prospects. V, we explore the diverse applications of spectrometers. Section IV delves into the important parameters of spectrometers, including spectral range, bandwidth, spectral resolution or spectral resolving power (SRP), étendue, and calibration from a theoretical standpoint. III, we construct a generalized reconstructive spectrometer model and introduce the principles behind spectral mapping, reconstruction, and imaging.
II, we present a systematic introduction to the fundamental principles, classifications, and typical applications of spectrometers in the fields of astronomy and remote sensing.
Spectrometers can be classified into several types, including prism, grating, Fourier transform (such as Michelson, Mach–Zehnder, and Sagnac interferometers), tunable filter (such as Fabry–Pérot, acousto-optic and liquid crystal tunable filters) spectrometers, as well as reconstructive spectrometers 2 (comprising spectral response and spectral-to-spatial mapping types). Within the realm of astronomical and remote sensing instruments, the optical spectrum analyzer (OSA), 1 or spectrometer, holds significant importance. It allows for the measurement of parameters such as wavelength, intensity, and profile, among others. A spectrometer is an instrument used for spectral analysis of optical signals, enabling the determination of the spectral composition of emitted, absorbed, or scattered optical radiation by substances.
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