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The next piece of the puzzle will involve explaining the cause of the dramatic, unprecedented trade wind acceleration.
A successful solar wind acceleration model should be able to explain all those solar winds.
Takigawa, A., Kamizuka, T., Tachibana, S. & Yamamura, I. Dust formation and wind acceleration around the aluminum oxide-rich AGB star W Hydrae. Sci.
We present the results of a comparison between out observations and the most recent version of the Lindau-Warsaw solar wind acceleration model.
In contrast to the polar coronal holes, the bulk of the solar wind acceleration must occur above 3 R⊙ for large low-latitude coronal holes at solar maximum.
The data obtained will be used for diagnostic purposes and modeling of solar wind acceleration, coronal plasma structures and various active phenomena in the solar corona.
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Estimation of possible wind accelerations along canyons using the derived database is also presented.
The occupant comfort is related to the motion perception under moderate winds, and quantified by the probability of exceeding threshold values of the across-wind acceleration at the top of the building.
For the setback and tapered models, although the across-wind acceleration is larger than that of the square model, the along-wind and torsional accelerations are smaller than those of the square model, resulting in smaller total rms acceleration response.
Measurements of surface pressures on 126 taps, overall forces, across-wind displacements and across-wind and along-wind accelerations were simultaneously carried out.
A control strategy is developed for application to a flexible laboratory structure excited by simulated wind forces for the purpose of minimizing along-wind accelerations.
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