| ... | @@ -22,12 +22,11 @@ I_{z} = I_{0} \cdot e^{-k_{d} \cdot z} |
... | @@ -22,12 +22,11 @@ I_{z} = I_{0} \cdot e^{-k_{d} \cdot z} |
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The extinction coefficient ($`k_{d}`$) is depending on the amount of Total Particulate Matter (TPM) in the water that varies over the season (described by the [cosine function](Data#suspended-solids)). The extinction coefficient is calculated from the TPM concentration using a simplified version of the function that is used by Los and Wijsman (2007), based on Van Gils and Tatman (2003).
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The extinction coefficient ($`k_{d}`$) is depending on the amount of Total Particulate Matter (TPM) in the water that varies over the season (described by the [cosine function](Data#suspended-solids)). The extinction coefficient is calculated from the TPM concentration using a simplified version of the function that is used by Los and Wijsman (2007), based on Van Gils and Tatman (2003).
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Los and Wijsman (2007) use the relation from Van Gils and Tatman (2003)
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Los and Wijsman (2007) use the relation from Van Gils and Tatman (2003)
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```math
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```math
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k_{d} = 0.24 + 0.036 \cdot TPM
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k_{d} = 0.24 + 0.036 \cdot TPM
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```
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```
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Where the background extinction is 0.25 m<sup>-1</sup> (including the extinction due to dissolved humic substances) and TPM is the concentration of suspended sediment particles (mg l<sup>-1</sup>)
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Where the background extinction is 0.24 m<sup>-1</sup> (including the extinction due to dissolved humic substances) and TPM is the concentration of suspended sediment particles (mg l<sup>-1</sup>)
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The average light ($`I_{avg}`$) is calculated by integration of the function over the whole water column divided over the waterdepth.
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The average light ($`I_{avg}`$) is calculated by integration of the function over the whole water column divided over the waterdepth.
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