{"refrec":{"BRefID":404400,"RR":"<b>Moradi, M.; Arabi, B.; Hommersom, A.; van der Molen, J.; Samimi, C.</b> (2024). Quality control tests for automated above-water hyperspectral measurements: Radiative Transfer assessment. <i>Isprs Journal of Photogrammetry and Remote Sensing 215</i>: 292-312. <a href=\"https://dx.doi.org/10.1016/j.isprsjprs.2024.07.011\" target=\"_blank\">https://dx.doi.org/10.1016/j.isprsjprs.2024.07.011</a>","BEntID":402191,"PublicFlag":1,"CheckedFlag":0,"wosflag":1,"vabbflag":1,"RefStringPartII":". <i>Isprs Journal of Photogrammetry and Remote Sensing 215</i>: 292-312. <a href=\"https://dx.doi.org/10.1016/j.isprsjprs.2024.07.011\" target=\"_blank\">https://dx.doi.org/10.1016/j.isprsjprs.2024.07.011</a>","DocTypID":8,"DocType":"Journal article","MarineFlag":0,"FreshFlag":0,"BrackishFlag":0,"TerrestrialFlag":0,"Authorstring":"Moradi, M.; Arabi, B.; Hommersom, A.; van der Molen, J.; Samimi, C.","OrigTitleTranslFlag":0,"Authorstringtrunc":"Moradi, M. <i>et al.</i>","Englishabstract":"<span style=\"color:rgb(31,31,31);\">Automated above-water hyperspectral observations are often subject to inaccuracies caused by instrument malfunction and environmental conditions. This study evaluates the influence of atmospheric and water surface conditions on above-water hyperspectral measurements through statistical methods and </span><a href=\"https://www.sciencedirect.com/topics/earth-and-planetary-sciences/radiative-transfer\"><span style=\"color:rgb(31,31,31);\">Radiative Transfer</span></a><span style=\"color:rgb(31,31,31);\"> (RT) modelling. Initially, we developed a general quality control method based on statistical assessment to detect the suspicious spectra. Subsequently, Radiative Transfer (RT) models were used to assess low light conditions, distortions in the spectral shape of above-water solar </span><a href=\"https://www.sciencedirect.com/topics/earth-and-planetary-sciences/downwelling\"><span style=\"color:rgb(31,31,31);\">downwelling</span></a><span style=\"color:rgb(31,31,31);\"> irradiance (</span><i>E<sub>S</sub></i><span style=\"color:rgb(31,31,31);\">(λ), mW m</span><sup>−2</sup><span style=\"color:rgb(31,31,31);\"> nm</span><sup>−1</sup><span style=\"color:rgb(31,31,31);\">) particularly those caused by intense </span><a href=\"https://www.sciencedirect.com/topics/earth-and-planetary-sciences/atmospheric-scattering\"><span style=\"color:rgb(31,31,31);\">atmospheric scattering</span></a><span style=\"color:rgb(31,31,31);\"> and/or reddish hue of dusk or dawn radiation, the effect of </span><a href=\"https://www.sciencedirect.com/topics/earth-and-planetary-sciences/atmospheric-humidity\"><span style=\"color:rgb(31,31,31);\">atmospheric humidity</span></a><span style=\"color:rgb(31,31,31);\"> and precipitation on the intensity and shape of spectra, and the influence of </span><a href=\"https://www.sciencedirect.com/topics/earth-and-planetary-sciences/sun-glint\"><span style=\"color:rgb(31,31,31);\">sun glint</span></a><span style=\"color:rgb(31,31,31);\"> and surface perturbations on sky (</span><i>L<sub>S</sub></i><span style=\"color:rgb(31,31,31);\">(λ), mW m</span><sup>−2</sup><span style=\"color:rgb(31,31,31);\"> nm</span><sup>−1</sup><span style=\"color:rgb(31,31,31);\"> sr</span><sup>−1</sup><span style=\"color:rgb(31,31,31);\">) and water surface (</span><i>L<sub>T</sub></i><span style=\"color:rgb(31,31,31);\">(λ), mW m</span><sup>−2</sup><span style=\"color:rgb(31,31,31);\"> nm</span><sup>−1</sup><span style=\"color:rgb(31,31,31);\"> sr</span><sup>−1</sup><span style=\"color:rgb(31,31,31);\">) radiances. The proposed methods were applied to the entire archive of automated above-water hyperspectral measurements collected every ten minutes from 2020 to 2022 at the Royal Netherland Institute for Sea Research (NIOZ) at Jetty Station (NJS) located in the Marsdiep </span><a href=\"https://www.sciencedirect.com/topics/earth-and-planetary-sciences/tidal-inlet\"><span style=\"color:rgb(31,31,31);\">tidal inlet</span></a><span style=\"color:rgb(31,31,31);\"> of the Duch </span><a href=\"https://www.sciencedirect.com/topics/earth-and-planetary-sciences/wadden-sea\"><span style=\"color:rgb(31,31,31);\">Wadden Sea</span></a><span style=\"color:rgb(31,31,31);\">, the Netherlands. The findings demonstrate that low light conditions are characterized by </span><i>E<sub>S</sub></i><span style=\"color:rgb(31,31,31);\">(λ)</span><sub>max</sub><span style=\"color:rgb(31,31,31);\">&nbsp;≤&nbsp;25 mW m</span><sup>−2</sup><span style=\"color:rgb(31,31,31);\"> nm</span><sup>−1</sup><span style=\"color:rgb(31,31,31);\">. Red-shifted or distorted spectra are indicated by a ratio of </span><i>E<sub>S</sub></i><span style=\"color:rgb(31,31,31);\">(4&nbsp;8&nbsp;0)/</span><i>E<sub>S</sub></i><span style=\"color:rgb(31,31,31);\">(6&nbsp;8&nbsp;0)&nbsp;≤&nbsp;1.0 and </span><i>E<sub>S</sub></i><span style=\"color:rgb(31,31,31);\">(λ</span><sub>max</sub><span style=\"color:rgb(31,31,31);\">)/ </span><i>E<sub>S</sub></i><span style=\"color:rgb(31,31,31);\">(8&nbsp;6&nbsp;5)&nbsp;≤&nbsp;1.25. High humidity/precipitation conditions are identified by the ratio of </span><i>E<sub>S</sub></i><span style=\"color:rgb(31,31,31);\">(9&nbsp;4&nbsp;0)/</span><i>E<sub>S</sub></i><span style=\"color:rgb(31,31,31);\">(8&nbsp;6&nbsp;5), which varies with the Solar </span><a href=\"https://www.sciencedirect.com/topics/earth-and-planetary-sciences/zenith-angle\"><span style=\"color:rgb(31,31,31);\">Zenith Angle</span></a><span style=\"color:rgb(31,31,31);\"> (SZA). Furthermore, significant sun glint and surface perturbations, such as whitecaps and foam, are indicated when the minimum ratio of </span><i>L<sub>T</sub></i><span style=\"color:rgb(31,31,31);\">(800&nbsp;nm-950&nbsp;nm)/</span><i>E<sub>S</sub></i><span style=\"color:rgb(31,31,31);\">(800&nbsp;nm-950&nbsp;nm)&nbsp;&gt;&nbsp;0.025 sr</span><sup>−1</sup><span style=\"color:rgb(31,31,31);\">, and the ratio of </span><i>L<sub>T</sub></i><span style=\"color:rgb(31,31,31);\">(850&nbsp;nm)/</span><i>E<sub>S</sub></i><span style=\"color:rgb(31,31,31);\">(850&nbsp;nm)&nbsp;≥&nbsp;0.025 sr</span><sup>−1</sup><span style=\"color:rgb(31,31,31);\">.</span>","AbstractOtherLang":null,"BibLvlCode":"AS","StandardTitle":"Quality control tests for automated above-water hyperspectral measurements: Radiative Transfer assessment","OrigTitleLangCode":"en","OrigTitleLangCodeExtended":"eng","OrigTitleLangID":15,"DateLastModified":{"date":"2024-12-10 01:33:17.368041","timezone_type":1,"timezone":"+01:00"},"UserAccessRight":null,"UserAccID":null,"AuthorKeywords":"<p style=\"margin-left:0px;\">Remote sensing; Ocean optics; Water quality; Coastal waters; Wadden sea","OtherDescriptors":null,"Notes":null,"AnaPub":2024,"MonPub":null,"DateUpdate":"2024-11-26","DateCreate":"2024-11-26","SecASFANote":null,"ConfID":null,"PeerRev":1,"VlizCoreFlag":1,"WoScode":null,"VABBcode":null,"OpenAcc":0,"DOI":"10.1016/j.isprsjprs.2024.07.011"},"refs":null,"anarec":{"AnaID":404400,"PubliDate":2024,"Pagination":"292-312","XtraPublOfAnaID":null,"ISBN":null,"Volume":"215","Issue":null,"BRefMon":null,"BRefMonRR":null,"BRefXtra":null,"BRefXtraRR":null,"SerBRefID":270870,"SerRR":"Isprs Journal of Photogrammetry and Remote Sensing. 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