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The results suggest that conventionally measured glass transitions originate from the broad amorphous gaps between lamellar stacks in these space-filling spherulitic systems.
Measured glass transition temperatures, i.e., 11.0 °C for PI and −0.7 °C for PB are both considerably high compared with those of 1,4-microstructure-rich analogues.
From simulations, the χ versus concentration plot shows the same trend as the experimentally measured glass transition temperature versus concentration plot.
From the measured glass transition temperature and the specific heat increments (ΔCp) at Tg, it was found that the P4MS dissolved more easily in the iPS rich-phase than did the iPS in the P4MS rich-phase.
Table 8 shows that the (calorimetrically measured) glass transition temperature depends strongly on the nature of the food components.
However, confined crystallization can only occur at a larger fPS-rich, though the measured glass transition temperature (Tg) is high for the PS block.
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Thermometers were installed in the sloped solar collector to measure glass, air, and absorption layer temperatures along the collector.
To simulate this multi-barrier repository scenario in the laboratory, several tests have been performed to measure glass dissolution rates of the simulated high-level nuclear waste glass, SON68, in the presence of COx claystone at 90 °C.
To do this take a large liquid measuring vessel (e.g. 2C measuring glass), fill it with water to a particular point (e.g. 1C) and then scoop the food you are trying to measure into the water.
They bought 20 kinds of wine and cocktail glasses at yard sales, aimed a loudspeaker at each and measured the glass's vibration.
The rate of oxygen uptake was measured in glass sample tubes into which microcathode oxygen electrodes were inserted.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com