This shows you the differences between two versions of the page.
Both sides previous revisionPrevious revisionNext revision | Previous revisionNext revisionBoth sides next revision | ||
tutorials:t20 [2019/08/13 17:56] – [Grain growth of supersaturated Fe-matrix - solute drag effect] pwarczok | tutorials:t20 [2023/08/18 13:13] – [Grain growth of pure Fe-matrix] pwarczok | ||
---|---|---|---|
Line 2: | Line 2: | ||
//This tutorial was tested on\\ | //This tutorial was tested on\\ | ||
- | MatCalc version 6.01 rel 1.003\\ | + | MatCalc version 6.03 rel 1.000\\ |
license: free\\ | license: free\\ | ||
database: mc_fe.tdb; mc_fe.ddb// | database: mc_fe.tdb; mc_fe.ddb// | ||
Line 35: | Line 35: | ||
Next, in the **'MS Evolution' | Next, in the **'MS Evolution' | ||
- | {{: | + | {{: |
Using **Calc > precipitation kinetics**, set up an isothermal simulation with an end-time of 3600 s (1 hour) and a temperature of 900°C. Click on **' | Using **Calc > precipitation kinetics**, set up an isothermal simulation with an end-time of 3600 s (1 hour) and a temperature of 900°C. Click on **' | ||
Line 71: | Line 71: | ||
{{: | {{: | ||
- | A further decrease of the grain rate can be observed, once the precipitate phase is present. On the first sight, one might get an impression that the effect of the precipitates is not that big. However, it must be remarked that the precipitates were created in this simulation and phase fraction of these has a minor value of 4e-6 after one hour, compared to around 4e-4 in equilibrium at this temperature. The difference in the grain sizes gets more and more significant, | + | A further decrease of the grain rate can be observed, once the precipitate phase is present. On the first sight, one might get an impression that the effect of the precipitates is not that big. However, it must be remarked that the precipitates were created in this simulation and phase fraction of these has a minor value of almost |