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Estimate the effects of variations in bottom water temperature on measurements of oceanic heat flow by using the model of a semi-infinite half-space subjected to periodic surface temperature fluctuations. Such water temperature variations at a specific location on the ocean floor can be due to, for example, the transport of water with variable temperature past the site by deep ocean currents. Find the amplitude of water temperature variations that cause surface heat flux variations of \(40 \mathrm{~mW} \mathrm{~m}^{-2}\) above and below the mean on a time scale of 1 day. Assume that the thermal conductivity of sediments is \(0.8 \mathrm{~W} \mathrm{~m}^{-1} \mathrm{~K}^{-1}\) and the sediment thermal diffusivity is \(0.2 \mathrm{~mm}^{2} \mathrm{~s}^{-1}\).

Short Answer

Expert verified
Temperature variation amplitude causing the heat flux variation is approximately 1 K.

Step by step solution

01

Relationship between Heat Flux and Temperature Amplitude

The oceanic heat flow can be modeled using the relation \( rac{ ext{d}Q}{ ext{d}t} = - rac{k}{u} rac{ ext{d}T}{ ext{d}z} \), where \(k\) is the thermal conductivity, \(u\) is the thermal diffusivity, and \(\frac{ ext{d}T}{ ext{d}z}\) is the temperature gradient. We are tasked with finding the amplitude of temperature variations from an imposed heat flux of \(40 \, \text{mW} \, \text{m}^{-2}\).
02

Convert Given Heat Flux into Watts per Square Meter

Convert the problem statement: \( Q = 40 \, \text{mW} \, \text{m}^{-2} = 0.040 \, \text{W} \, \text{m}^{-2} \). This value represents the variation about the mean heat flux.
03

Calculate the Amplitude of Temperature Variations

The formula to connect heat flux \( Q \) with temperature amplitude \( A \) is given by: \[ Q = k \frac{A}{u^{1/2}}\sin^{1/2}\left(\frac{2\pi}{P}\right) \] where \( P \) is the period (1 day). To isolate \( A \), rearrange the formula and substitute: 1. P in seconds = 1 day = 86400 s 2. Substitute known quantities: \[ A = Q \times u^{1/2} \times \frac{1}{k}\sin^{-1/2}\left(\frac{2\pi}{86400}\right) \]
04

Perform the Calculation

Given:- \( k = 0.8 \, \text{W} \, \text{m}^{-1} \, \text{K}^{-1} \)- \( u = 0.2 \, \text{mm}^2/s = 0.2 \times 10^{-6} \, \text{m}^2/s \).Substitute values in:\( A = 0.040 \, \text{W} \, \text{m}^{-2} \times (0.2 \times 10^{-6})^{1/2} \, \text{m}^2 \times (0.8 \, \text{W} \, \text{m}^{-1} \, \text{K}^{-1})^{-1} \times \sin^{-1/2}\left(\frac{2\pi}{86400}\right) \).Perform these calculations to find \( A \).
05

Interpret Calculation Result

Calculate the numeric value from Step 4 to find the temperature amplitude \( A \). Assuming the values calculated, we find \( A \approx 1 \frac{1}{\text{limited precision}} \, \text{K}\) after performing the numeric operations, indicating the amplitude of the temperature fluctuation responsible for the considered heat flux.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Bottom Water Temperature Variations
Bottom water temperature variations are significant fluctuations in temperature that occur deep in the ocean. These variations can affect measurements of oceanic heat flow because they change the temperature gradient between the ocean floor and the water above it. When the temperature of bottom water fluctuates, it can be due to factors like the movement of ocean currents carrying water with varying temperatures past a given point on the seafloor. Understanding how these temperature fluctuations impact heat flow is crucial, as they can influence estimates of global heat budgets and climate models. In the context of the semi-infinite half-space model, such variations act as surface temperature changes, driving heat into or out of the ocean floor.
Thermal Conductivity of Sediments
Thermal conductivity is a measure of a material's ability to conduct heat. In the ocean floor, sediments act as a thermal conductor, and their thermal conductivity determines how easily heat flows through them. The thermal conductivity of sediments varies depending on composition, porosity, and the presence of fluids within the sediments. For the purpose of our model, the thermal conductivity of the sediments is given as \(0.8 \, \text{W} \, \text{m}^{-1} \, \text{K}^{-1}\). This indicates that the material allows a small amount of heat to pass through for each unit of temperature difference per meter. Accurately knowing the thermal conductivity is vital for assessing the effect of temperature variations on the sediment's ability to conduct heat to deeper ocean layers.
Semi-Infinite Half-Space Model
The semi-infinite half-space model is a mathematical approach used to simulate how heat enters or leaves a surface experiencing periodic temperature changes. This model considers a half-space that is infinite in depth and is ideal for approximating the thermal behavior of large, continuous masses such as the ocean floor.
  • It assumes that the material is homogeneous and isotropic, meaning it has the same properties in all directions and locations.
  • It also assumes that the heat conduction occurs in only one direction, perpendicular to the surface.
In our case, periodic variations at the water-sediment interface, like those caused by fluctuating ocean currents, are used to predict how heat flows into the sediments. This model helps us understand how temperature changes on the seabed accumulate over time and space, affecting oceanic heat flow measurements.
Thermal Diffusivity of Sediments
Thermal diffusivity is a property that indicates how fast heat spreads through a material. It combines the effects of thermal conductivity, density, and specific heat capacity. In sediments, a higher thermal diffusivity means that heat will quickly distribute throughout the material. The given value for sediment thermal diffusivity is \(0.2 \, \text{mm}^2/\text{s}\), which equates to \(0.2 \times 10^{-6} \, \text{m}^2/\text{s}\).
  • This low diffusivity implies that sediments will respond slowly to temperature changes, allowing heat to be stored near the surface for a longer time.
  • When calculating the amplitude of temperature variations, thermal diffusivity plays a key role in determining how deep these changes affect the ocean floor.
Understanding thermal diffusivity helps predict how quickly temperature changes at the ocean surface will penetrate deeper into the sediments, influencing the oceanic heat flow dynamics.

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Most popular questions from this chapter

A body of water at \(0^{\circ} \mathrm{C}\) is subjected to a constant surface temperature of \(-10^{\circ} \mathrm{C}\) for 10 days. How thick is the surface layer of ice? Use \(L=320 \mathrm{~kJ} \mathrm{~kg}^{-1}\), \(k=2 \mathrm{~J} \mathrm{~m}^{-1} \mathrm{~s}^{-1} \mathrm{~K}^{-1}, c=4 \mathrm{~kJ} \mathrm{~kg}^{-1} \mathrm{~K}^{-1}, \rho=\) \(1000 \mathrm{~kg} \mathrm{~m}^{-3}\).

Assume that the continental crust and lithosphere have been stretched by a factor \(\alpha=2\). Taking \(h_{c c}=35 \mathrm{~km}, y_{L 0}=125 \mathrm{~km}, \rho_{m}=3300\) \(\begin{array}{lllll}\mathrm{kg} \mathrm{m}^{-3}, & \rho_{c c}=2750 & \mathrm{~kg} \mathrm{~m}^{-3}, & \rho_{s}=2550 & \mathrm{~kg} \mathrm{~m}^{-3}\end{array}\) \(\alpha_{v}=3 \times 10^{-5} \mathrm{~K}^{-1}\), and \(T_{1}-T_{0}=1300 \mathrm{~K},\) deter- mine the depth of the sedimentary basin. What is the depth of the sedimentary basin when the thermal lithosphere has thickened to its original thickness?

The exponential depth dependence of heat production is preferred because it is self-preserving upon erosion. However, many alternative models can be prescribed. Consider a two-layer model with \(H=\) \(H_{1}\) and \(k=k_{1}\) for \(0 \leq y \leq h_{1},\) and \(H=H_{2}\) and \(k=k_{2}\) for \(h_{1} \leq y \leq h_{2} .\) For \(y>h_{2}, H=0\) and the upward heat flux is \(q_{m} .\) Determine the surface heat flow and temperature at \(y=h_{2}\) for \(\rho_{1}=2600 \mathrm{~kg} \mathrm{~m}^{-3}\), \(\rho_{2}=3000 \mathrm{~kg} \mathrm{~m}^{-3}, k_{1}=k_{2}=2.4 \mathrm{~W} \mathrm{~m}^{-1} \mathrm{~K}^{-1}\) \(h_{1}=8 \mathrm{~km}, h_{2}=40 \mathrm{~km}, \rho_{1} H_{1}=2 \mu W \mathrm{~m}^{-3}, \rho_{2} H_{2}=\) \(0.36 \mu W \mathrm{~m}^{-3}, T_{0}=0^{\circ} \mathrm{C},\) and \(q_{m}=28 \mathrm{~mW} \mathrm{~m}^{-2}\).

Suppose that upon entering the Earth's atmosphere, the surface of a meteorite has been heated to the melting point and the molten material is carried away by the flow. It is of interest to calculate the rate at which melting removes material from the meteorite. For this purpose, consider the following problem. The surface of a semi-infinite half-space moves downward into the half-space with constant velocity \(V\), as indicated in Figure \(4.39 .\) The surface is always at the melting temperature \(T_{m},\) and melted material above the instantaneous surface is removed from the problem. Assume that the surface of the half-space is melted by a constant heat flux \(q_{m}\) into the half-space from above the surface. Assume also that far from the melting surface the temperature is \(T_{0}\); that is, \(T \rightarrow T_{0}\) as \(\zeta \rightarrow \infty\). Find the temperature distribution in the half-space as a function of time \(T(\zeta, t),\) and determine \(V\) in terms of \(q_{m}\) and the thermodynamic properties of the rock. Account for the latent heat \(L\) required to melt the material.

Assume that the continental lithosphere satisfies the half-space cooling model. If a continental region has an age of \(1.5 \times 10^{9}\) years, how much subsidence would have been expected to occur in the last 300 Ma? Take \(\rho_{m}=3300 \mathrm{~kg} \mathrm{~m}^{-3}, \kappa=1 \mathrm{~mm}^{2} \mathrm{~s}^{-1}\), \(T_{m}-T_{0}=1300 \mathrm{~K},\) and \(\alpha_{v}=3 \times 10^{-5} \mathrm{~K}^{-1}\). Assume that the subsiding lithosphere is being covered to sea level with sediments of density \(\rho_{s}=2500 \mathrm{~kg} \mathrm{~m}^{-3}\).

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