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The speed of structure generation depends on the size of the molecular fragments.
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When multiple triple flames are in close proximity, the bulk propagation speed of the structure can be even faster due to additional streamline divergence.
Recent developments in experimental and computational aspects of NMR spectroscopy have had a significant impact on the accuracy and speed of macromolecular structure determination in solution, particularly with regard to systems of high complexity (such as protein complexes).
The results of charge collection efficiency and charge collection speed of these structures are discussed.
Based on the tests data, the physical process of dynamic ice forces in crushing failure was probed, by analysis of mechanical behaviour of ice under compressive loading related to relative loading speed of ice-structure interaction.
With the assistance of experimental data, such as thermodynamics, NMR spectra, and chemical and enzymatic mapping, computational predictions can greatly increase the speed for discovery of structure (8− 15).
In this paper, we obtain measures of uncertainties in the estimation of the wind speeds upwind of structures.
The propagation speed of the WN4 structure estimated by this method is about 4.3°/h in low solar activity and about 3.2°/h in high solar activity.
The effects of the reactant concentration and rotation speed of the dynamic structure on the crystal size and morphology were investigated.
The eastward propagation speed of the WN4 structure estimated from local time difference of NmF2 is found to be about 4.3°/h in low solar activity period and about 3.2°/h in high solar activity period.
We obtained a formula that describes the propagation speed of the helical structure, which is proportional to the DMI strength but is not influenced by the strength of the exchange interaction.
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