The 2014 2nd International Conference on Systems and Informatics (ICSAI 2014) 2014
DOI: 10.1109/icsai.2014.7009407
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Laboratory spectral calibration and radiometric calibration of hyper-spectral imaging spectrometer

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Cited by 16 publications
(11 citation statements)
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“…The second limitation is that of calibration drift. Calibration of such systems is generally performed using known spectral sources such as a xenon, mercury or sodium lamp [31,32]. Spectral features can be identified from instrument output, and these are used to establish the range and resolution of the instrument.…”
Section: Introductionmentioning
confidence: 99%
“…The second limitation is that of calibration drift. Calibration of such systems is generally performed using known spectral sources such as a xenon, mercury or sodium lamp [31,32]. Spectral features can be identified from instrument output, and these are used to establish the range and resolution of the instrument.…”
Section: Introductionmentioning
confidence: 99%
“…The goal of radiometric calibration is to correctly convert the raw data from sensor count to spectral radiance so that the measurements are comparable to data from other instruments. As radiometric calibration relies on the wavelength calibration [8], the wavelength calibration must be performed first.…”
Section: Radiometric Calibrationmentioning
confidence: 99%
“…By changing the wavelength of the monochromatic collimation light each time, the spectral response curve of each channel is acquired (Figure 8). The SRF can be well-approximated by a Gaussian function with appropriate parameters as in Equation (1) [23]. SRF(λ)=A0+A1exp[(λλ0)22σ2] where λ0 is the center wavelength and full width at half maximum (FWHM) is calculated as FWHM=22ln2σ.…”
Section: Laboratory Calibrationmentioning
confidence: 99%