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Medspiration – System Requirements Document - Data User Element

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<strong>Medspiration</strong><br />

MED-SOC-RS-001_1<br />

<strong>System</strong> <strong>Requirements</strong> <strong>Document</strong><br />

Issue F<br />

measured by an infrared radiometer operating in the 10 – 12 µm waveband.<br />

Physically it represents the temperature of the water at a depth of approximately 10 –<br />

20 µm.<br />

• SSTsubskin represents the temperature at the base of the thermal skin layer. The<br />

thermal skin layer is a region less than 1 mm deep in which the convective exchange<br />

of heat by turbulent mixing is inhibited by the proximity of the sea surface, so that the<br />

net outward flow of heat through the surface creates a steep reduction of temperature<br />

towards the surface. Below the skin layer, turbulent processes ensure that the<br />

temperature is nearly uniform over a depth of at least a few centimetres. By<br />

definition within GHRSST-PP this corresponds to the SSTsubskin temperature. In<br />

practice SSTsubskin is assumed to be approximately equal to the radiometric<br />

temperature measured by a microwave radiometer operating in the 6-11 GHz<br />

frequency band, although the relationship is not exact or fully known.<br />

• SSTdepth is the generic term used to represent the temperature measured by a<br />

contact thermometer within the upper few metres of the water column and generally<br />

referred to as the “bulk” SST. If the water column below the skin layer is uniform<br />

(typically the case at night and when wind mixing is strong) then SSTdepth is the<br />

same as SSTsubskin, irrespective of the actual depth of the measurement (see<br />

Figure 2-1a). However, when daytime solar shortwave radiation penetrates to heat<br />

the water below the skin layer, and if wind mixing is weak, stable stratification<br />

develops in the upper few metres of the water column, in which the temperature<br />

increases towards the sea surface (apart from the cool skin layer which lies right at<br />

the surface - see Figure 2-1b). This phenomenon is called a diurnal thermocline.<br />

When it occurs a measurement of SSTdepth, made from a buoy or ship-mounted<br />

thermometer which does not precisely specify the sampling depth, is of limited value.<br />

A diurnal thermocline almost always collapses to a uniform temperature some time<br />

after sunset when surface cooling removes the excess heat. Under calm conditions,<br />

however, it may take several hours for the diurnal thermocline to decay entirely.<br />

• SSTfnd is defined within GHRSST-PP as the temperature at the base of the diurnal<br />

thermocline. It is so named because it represents the foundation temperature on<br />

which the diurnal thermocline develops during the day. SSTfnd changes only<br />

gradually along with the upper layer of the ocean, and by definition it is independent<br />

of skin SST fluctuations due to wind- and radiation-dependent diurnal stratification or<br />

skin layer response. It is therefore updated at intervals of 24 hrs. SSTfnd<br />

corresponds to the temperature of the upper mixed layer which is the part of the<br />

ocean represented by the top-most layer of grid cells in most numerical ocean<br />

© 2004 SOC Page 15 of 193

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