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Turbidity in the southern Irish Sea

机译:爱尔兰南部海域的浊度

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This paper presents new in situ optical and associated measurements from 85 stations in the central and southern Irish Sea. There is a strong linear relationship between the irradiance reflectance R-A in the orange-red part of the spectrum (580-680 nm) and the diffuse attenuation coefficient, K, for white light: K = 0.05 + 0.26 R-A, where K is in m(-1) and R-A has been corrected to just above-surface reflectance and expressed as a percentage. The significance of this result is that this particular reflectance can be measured by the advanced very high resolution radiometer on board the NOAA series of satellites. In principle, therefore, cloud cover permitting, the transparency of the Irish Sea to sunlight, can be mapped from space. This result is shown to be consistent with a simple optical model in which light scattering is principally by mineral suspended solids, and light absorption is by water, mineral suspended solids and chlorophyll. Best fit between model and observations is achieved with a specific scattering coefficient of 0.5 m(2) g(-1). The measurements were made during four cruises, at different times of year and across the range of turbidity found in the Irish Sea. The geographical distribution of suspended sediments confirms the presence, previously inferred from satellite imagery, of two separate turbidity maxima, one off Wicklow Head, the other off Anglesey. These correspond to the areas of strongest tidal currents. Yellow substance was found in highest concentration in a band along the Irish coast. Chlorophyll concentrations were generally low during these cruises. A residual problem is that a direct comparison of in situ reflectance and satellite measured reflectance possible on one of the cruises shows a serious discrepancy, although on average there appears to be a good agreement between satellite and in situ reflectance. (C) 2002 Elsevier Science Ltd. All rights reserved. [References: 23]
机译:本文介绍了来自爱尔兰中部和南部海域85个站点的新的原位光学和相关测量结果。光谱的橙红色部分(580-680 nm)中的辐照度反射率RA与白光的漫射衰减系数K之间存在很强的线性关系:K = 0.05 + 0.26 RA,其中K以m为单位(-1)和RA已被校正为刚好高于表面反射率并以百分比表示。该结果的意义在于,可以通过NOAA系列卫星上的先进超高分辨率辐射计测量该特定的反射率。因此,原则上可以从太空中绘制云层覆盖范围,即爱尔兰海对阳光的透明性。该结果表明与简单的光学模型是一致的,在该光学模型中,光的散射主要是由矿物悬浮物引起的,而光的吸收是由水,矿物悬浮物和叶绿素引起的。模型与观测值之间的最佳拟合是通过0.5 m(2)g(-1)的特定散射系数实现的。在一年中的不同时间以及在爱尔兰海中发现的浑浊范围内的四次航行中进行了测量。悬浮沉积物的地理分布确定了先前从卫星图像推断出的两个单独的浊度最大值,一个位于威克洛头附近,另一个位于安格尔西附近。这些对应于最强的潮流区域。在爱尔兰海岸的一条带中发现了最高浓度的黄色物质。在这些航行中,叶绿素浓度通常较低。一个剩余的问题是,在一次巡航中可能将原位反射率和卫星测得的反射率直接进行比较显示出严重的差异,尽管平均而言,卫星和原位反射率之间似乎有很好的一致性。 (C)2002 Elsevier ScienceLtd。保留所有权利。 [参考:23]

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