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Open image in new window Fig. 5 Time mean pressure profiles along the axial height of the dipleg.
The time mean pressure profiles could be divided into three regions according to the local pressure gradient or the linear pressure distribution.
For this submerged dipleg, the typical time mean pressure profiles along the axial direction were characterized by a progressively increasing pressure from top to bottom, as shown in Fig. 5.
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Simulations results with the SST turbulence model regarding mean velocity, temperature and pressure profiles in the shell side have been analysed and compared with those provided by HTRI Xchanger Suite®.
For these two wells, the bottom hole pressure (BHP) predictions were made for the entire duration between 2000 and 2008, which simply means what the pressure profile would have been if these wells existed at these locations.
Characteristics of hydrostatics and the gas law equation mean that relatively small systematic differences in temperature versus pressure profiles can integrate at high altitudes to very large differences in density versus altitude profiles.
Figure 5 Numerical calculated pressure profiles.
Fig. 1 Pressure profiles inside some protoplanets.
Pressure profiles exhibit mixed results.
Mean pressure coefficient = Mean pressure 1 12 2 ρ v 2 (1).
Figure 20 shows pressure profiles in three cases.
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