Posted by Krysten on Friday, March 5, 2010 at 6:06am.
If you had posted these questions separately, an answer might have been obtained sooner. I can only help with some of your questions. Oceanography is not my field.
(a) For the first one, solve this "Beer's law" equation for k:
exp(-kL) = 7.3*10^13/1.6*10^17 = 4.56*10^-4
kL = 7.7
k = 7.7/16 = 0.48 m^-1
This assumes the sun is overhead. It usually isn't.
(b) Use the same equation, but the lower value of k. Use the definition of the the "euphotic zone" (whatever that is) to solve for L
At extreme depths, Beer's law may not apply because scattering becomes important. You also need to know the elevation angle of the sun.
I can only guess that we are talking about the decay constant in I = Io e^-kx
Where for example :
Io = 1.6 * 10^17 *10^4 photons/m^2s
and
i at 16 m = 7.3 * 10^13 * 10^4 = 1.6 * 10^17 * 10^4 * e^-k(16)
4.56 *10^-4 = e^-16k
ln 4.56 -4 ln10 = -16 k
1.517 - 9.210 = -7.693 =16 k
k = 0.481/m
For the second part I do not know how dark it is when we say the euphotic zone ends. I am sure the irradiance for that is defined in whatever text the student is using.
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