2013
DOI: 10.1017/s0954102013000175
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Satellite-derived UV climatology at Escudero Station, Antarctic Peninsula

Abstract: Abstract:We have used data

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Cited by 12 publications
(11 citation statements)
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“…4a). This is similar to the range of CMF EUV (0.3 to 0.7) obtained at the Escudero station located near the King Sejong station (Cordero et al, 2013). For all cloudy conditions, the CMF EUV also apparently decreases as SZA becomes higher, averagely from 0.60 to 0.31 (Fig.…”
Section: Sza (Degree)supporting
confidence: 85%
“…4a). This is similar to the range of CMF EUV (0.3 to 0.7) obtained at the Escudero station located near the King Sejong station (Cordero et al, 2013). For all cloudy conditions, the CMF EUV also apparently decreases as SZA becomes higher, averagely from 0.60 to 0.31 (Fig.…”
Section: Sza (Degree)supporting
confidence: 85%
“…However, over snow-covered surfaces the OMI-derived dose is generally lower than the ground-based measurement because the OMI algorithm uses climatological surface albedo that may then be lower than the actual effective surface albedo [42] , [43] . Part of the problem is that a portion of the observed reflectivity may be incorrectly interpreted as cloud cover, which reduces the estimated irradiance [3] .…”
Section: Methodsmentioning
confidence: 99%
“…Although the latter may significantly modulate the surface UV, in Antarctica the load of aerosols is extremely low [1] . Moreover, while heavily overcast conditions can reduce surface UV irradiance up to 90% in the Antarctic Peninsula [2] , [3] , the role of clouds is less important on the Antarctic plateau. Therefore, surface UV in Antarctica is driven by ozone and by albedo.…”
Section: Introductionmentioning
confidence: 99%
“…An improved understanding of the radiation is therefore helpful to determine the impact of current and future changes on the climate in Antarctica. Angular distribution of solar radiance and its spectral characteristics are key radiative quantities to study the impact of climate changes in Antarctica (Cordero et al 2013(Cordero et al , 2014. These quantities and the absorption characteristics of snow determine how much radiation is reflected back to space and how much snow melts should temperatures rise.…”
Section: Progress In the Measurements Of Sky Luminance And Sky Radiancementioning
confidence: 99%