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A model of diffuse attenuation of downwelling irradiance for ecosystem models

机译:生态系统模型的下流辐照度扩散衰减模型

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Estimation of the underwater attenuation of light is important to ecosystem modellers, who require information on Photosynthetically Available Radiation (PAR), and on the euphotic depth for calculation of primary production. Characterisation of these processes can be achieved by determining the diffuse attenuation coefficient of PAR , KPAR . A review of bio-optical models- of the spectral diffuse attenuation coefficient for downwelling irradiance, Kd, is presented and stresses the necessity for a better knowledge and parameterization of these coefficients.rnIn the second part of this work, radiative transfer simulations were carried out to model K^^ the spectral diffuse attenuation of downwelling irradiance averaged over the euphotic depth Zl% (depth where the downwelling irradiance isrn1% of its surface value). This model takes into account the effects of varying sun zenith angle and cloud cover and needs absorption and backscattering coefficients (the inherent optical properties, IOPs) as input. It provides average and maximum relative errors of 1% and 5% respectively, for sun zenith angles [0°-50°] and of 1.7% and 12% respectively at higher sun zenith angles. A relationship was established between K^^ at a single wavelength (590nm) and KPAR atrnZPAm% (where PAR is 1% of its value at the surface) which allows for a direct expression of KPARZPARl% in terms ofrninherent optical properties, sun angle and cloudiness. This model provides estimates of KPAR within 25% (respectively 40%) relative errors respectively with a mean relative error less than 7% (respectively 9%) for sun zenith angles ranging from 0° to 50° (respectively higher than 50°). A similar method is applied to derive a model for the diffuse attenuation of photosynthetically usable radiation, KPURZPUm% , with similar performance.
机译:水下光衰减的估计对于生态系统建模者很重要,他们需要有关光合有效辐射(PAR)的信息以及关于一次生计算的共沸深度的信息。通过确定PAR,KPAR的扩散衰减系数,可以表征这些过程。提出了生物光学模型-向下辐射辐照度的光谱扩散衰减系数Kd的研究,并强调了对这些系数的更好了解和参数化的必要性。rn在这项工作的第二部分,进行了辐射传输模拟为了模拟K ^^,在整个共光深度Zl%(下沉辐照度为其表面值的1%处的深度)处平均下沉辐照度的光谱扩散衰减。该模型考虑了太阳天顶角和云量变化的影响,并且需要吸收系数和后向散射系数(固有光学特性,IOP)作为输入。对于太阳天顶角[0°-50°],它提供的平均和最大相对误差分别为1%和5%;在更高的太阳天顶角下,其分别提供的相对误差为1.7%和12%。在单个波长(590nm)处的K ^^与KPAR atrnZPAm%(其中PAR是其在表面的值的1%)之间建立了关系,这允许就固有的光学性质,太阳角和浑浊。该模型提供的KPAR估计分别在25%(分别为40%)的相对误差范围内,而从0°到50°(分别高于50°)的太阳天顶角的平均相对误差小于7%(分别为9%)。应用类似的方法来推导具有类似性能的光合可用辐射的扩散衰减KPURZPUm%的模型。

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