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<h3>Sea Surface Temperature (SST): A Detailed Mathematical Description</h3>
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To understand Sea Surface Temperature (SST) mathematically, we must view it as the thermodynamic result of the energy balance at the interface between the ocean and the atmosphere.
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<h3>Governing Thermodynamic Description of Sea Surface Temperature</h3>
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To understand Sea Surface Temperature (SST) mathematically, we must view it as the thermodynamic result of the energy balance at the
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interface between the ocean and the atmosphere. In physical oceanography, SST is not a single value but a vertical profile. We differentiate
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between the Skin Temperature \(\text{SST}_{\text{skin}}\) and the Bulk Temperature \(\text{SST}_{\text{bulk}}\).
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<h4>Temperature as a Prognostic Variable</h4>
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The ocean temperature field is a continuous function of space and time:
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$$T = T(x, y, z, t)$$
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where,
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<ul>
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<li>\(x, y\) are horizontal coordinates,</li>
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<li>\(z\) is vertical depth (positive downward),</li>
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<li>\(t\) is time.</li>
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</ul>
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Temperature evolution in the ocean is governed by energy conservation.
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</div>
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In physical oceanography, SST is not a single value but a vertical profile. We differentiate between the **Skin Temperature** () and the **Bulk Temperature** ().
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---
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## 1. The Governing Thermodynamic Equation
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The rate of change of temperature () in the upper ocean layer (the mixed layer) is governed by the conservation of heat energy. The heat budget equation for a water column of depth is:
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Where:
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* : Density of seawater ().
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* : Specific heat capacity of seawater ().
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* : Net surface heat flux.
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* : Heat loss/gain due to horizontal advection ().
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* : Vertical diffusion or entrainment at the base of the mixed layer.
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---
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## 2. The Net Surface Heat Flux ()
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<h4>Heat Conservation Equation (First Law of Thermodynamics)</h4>
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The local rate of change of temperature is governed by the heat equation:
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The is the most critical component for SST. It is the sum of four distinct flux terms:
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$$
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\rho c_p \frac{\partial T}{\partial t}
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= - \nabla \cdot \mathbf{F}_{\text{heat}} + Q
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$$
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### A. Shortwave Radiation ()
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where:
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This is the solar energy absorbed by the ocean. It depends on the solar constant, albedo (), and solar zenith angle ().
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<ul>
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<li>\(\rho\) is seawater density,</li>
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<li>\(c_p\) is specific heat capacity,</li>
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<li>\(\mathbf{F}_{\text{heat}}\) is the heat flux vector,</li>
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<li>\(Q\) represents internal heat sources (usually negligible near the surface).</li>
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</ul>
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<h4>Decomposition of Heat Flux</h4>
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The heat flux consists of advective and diffusive components:
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However, not all stays at the surface; it penetrates the water column according to **Beer’s Law**:
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$$
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\mathbf{F}_{\text{heat}}
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= \rho c_p \mathbf{u} T * k \nabla T
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$$
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where:
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<ul>
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<li>\(\mathbf{u}\) is the fluid velocity,</li>
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<li>\(k\) is thermal conductivity (or turbulent diffusivity).</li>
This boundary condition couples ocean thermodynamics to the atmosphere.
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* : Stanton number (transfer coefficient for heat).
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---
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<h4>Formation of the Skin Layer</h4>
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In the uppermost micrometers, turbulent mixing vanishes and molecular diffusion dominates. Under quasi-steady conditions:
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## 3. The "Cool Skin" Phenomenon
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$$
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\frac{\partial}{\partial z} \left( k \frac{\partial T}{\partial z} \right)= 0
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$$
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Because heat loss () occurs exactly at the surface, while heat gain () is distributed through depth, the very top layer (the "skin") is usually cooler than the water 10 cm below. This is described by the **Fourier Law of Conduction** in the molecular sublayer:
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which integrates to a linear gradient:
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* : Thickness of the molecular sublayer ().
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* : Thermal conductivity of water.
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---
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## 4. Summary Table of Variables
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| Variable | Description | Typical Units |
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| --- | --- | --- |
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| | Sea Surface Temperature | or |
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| | Latent Heat (Evaporation) | |
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| | Sensible Heat (Conduction) | |
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| | Surface Wind Speed | |
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| | Albedo (Reflectivity) | Dimensionless |
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---
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## 5. Why this matters for your research
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If you are applying to the research centers mentioned earlier (like **IITM** or **INCOIS**), you will likely deal with **Coupled Models**. In these models, the SST is the "boundary condition." If the math in your model incorrectly calculates (evaporation), your Monsoon predictions will fail.
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**Would you like me to explain how these equations are discretized for use in numerical climate models like WRF or ROMS?**
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