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The central pressure is in the range of 50 100 million atmospheres (about 50 100 megabars).
From diameters and masses, average values of the stellar density can be calculated and thence the central pressure.
Based on this analysis, it is shown that the central pressure deficit, Δp, contributes the most to the wind speed.
(G is the universal gravitational constant). From diameters and masses, average values of the stellar density can be calculated and thence the central pressure.
The central pressure of the storm has to drop at the rate of one millibar per hour for at least 24 hours.
On the basis of the 65-year dataset, the typhoon parameters of these three categories, including the central pressure and the maximum wind speed, were investigated.
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The central pressures simulated using the coupled model were higher than the central pressures simulated using the uncoupled model for all of the typhoons.
During the intensification phase, in contrast, the central pressures simulated using the uncoupled model were much higher than the best-track central pressures for T1109 (Figure 9b).
The central pressures for T1106 (Figure 9a) and T1221 (Figure 9d) simulated using the uncoupled model were lower than the RSMC-Tokyo best-track central pressures, particularly during the mature phase.
The coupled model simulated sea surface cooling and the resultant increases in the central pressures caused by the passages of the typhoons reasonably well.
The simulated sea surface cooling induced by the typhoon began to have an impact on the simulated central pressure during the intensification phase for all four typhoons.
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