2020
DOI: 10.1504/ijspacese.2020.109745
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Radiance enhancement and shortwave upwelling radiative flux methods for efficient detection of cloud scenes

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Cited by 6 publications
(11 citation statements)
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“…respectively. The real part of the complex error function K(x, y) also known as the Voigt function, occurs in great diversity in astrophysical spectroscopy, space science, neutron physics, plasma physics and statistical communication theory, as well as in some areas in mathematical physics and engineering associated with multi-dimensional analysis of spectral harmonics [4][5][6][7][8][9][10][11][12][13][14][15][16]. For example, the Voigt function is a fundamental component of the line-by-line (LBL) radiative transfer modeling for the analysis of planetary atmospheres [5][6][7].…”
Section: Introductionmentioning
confidence: 99%
“…respectively. The real part of the complex error function K(x, y) also known as the Voigt function, occurs in great diversity in astrophysical spectroscopy, space science, neutron physics, plasma physics and statistical communication theory, as well as in some areas in mathematical physics and engineering associated with multi-dimensional analysis of spectral harmonics [4][5][6][7][8][9][10][11][12][13][14][15][16]. For example, the Voigt function is a fundamental component of the line-by-line (LBL) radiative transfer modeling for the analysis of planetary atmospheres [5][6][7].…”
Section: Introductionmentioning
confidence: 99%
“…Alongside with conventional methods based on MODIS and Google cloud database that provides precise and efficient probabilistic approach in determination of the multi-layered cloud masking [15,16], the infra-red (IR) remote sensing is another approach for detection of clouds [8,[17][18][19]. In particular, in our recent publications we have described a new method for detection of cloud scenes based on the radiance enhancement (RE) method [18,19].…”
Section: Introductionmentioning
confidence: 99%
“…Alongside with conventional methods based on MODIS and Google cloud database that provides precise and efficient probabilistic approach in determination of the multi-layered cloud masking [15,16], the infra-red (IR) remote sensing is another approach for detection of clouds [8,[17][18][19]. In particular, in our recent publications we have described a new method for detection of cloud scenes based on the radiance enhancement (RE) method [18,19]. Despite some drawbacks of the RE method such as lower resolution and difficulties to distinguish multi-layered clouds, its application, nevertheless, may be advantageous especially when remote sensing is provided from the space-orbiting IR micro-spectrometer like Argus 1000 [18,19].…”
Section: Introductionmentioning
confidence: 99%
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“…We have shown recently that the datasets of the upwelling radiance collected from space remote sensor can also be used for efficient detection of cloud scenes by using the Radiance Enhancement method [11][12][13][14]. Specifically, the RE method utilizes the line-by-line radiative transfer model GEN-SPECT [15] in order to match the synthetic radiance with observed radiance by incrementing or decrementing several variables like concentration of gases, zenith angle, deviation of the nadir angle, etc.…”
Section: Introductionmentioning
confidence: 99%