Triple Point Based Parent Phase Reconstruction edit page

In this section we discuss triple point based parent grain reconstruction at the example of a titanium alloy. Lets start by importing a sample data set

The data set contains 99.8 percent alpha titanium and 0.2 percent beta titanium. Our goal is to reconstuct the original beta phase. The original grain structure appears almost visible for human eyes. Our computations will be based on the Burgers orientation relationship

that alligns (110) plane of the beta phase with the (0001) plane of the alpha phase and the [1-11] direction of the beta phase with the [2110] direction of the alpha phase.

Note that all MTEX functions for parent grain reconstruction expect the orientation relationship as parent to child and not as child to parent.

## Setting up the parent grain reconstructor

Grain reconstruction is guided in MTEX by a variable of type parentGrainReconstructor. During the reconstruction process this class keeps track about the relationship between the measured child grains and the recovered parent grains. In order to set this variable up we first need to compute the initital child grains from out EBSD data set.

As our reconstruction will be based on triple junctions we compute the child grains using the option removeQuadruplePoints which turns all quadruple junctions into 2 triple junctions. Furthermore, we choose a very small threshold of 1.5 degree for the identification of grain boundaries to avoid alpha orientations that belong to different beta grains get merged into the same alpha grain.

Now we are ready to set up the parent grain reconstruction job.

## Compute parent orientations from triple junctions

In present datas set we have very little and unreliable parent measurements. Therefore, we use triple junctions as germ cells for the parent parent grains. In a first step we identify triple junctions that have misorientations that are compatible with a common parent orientation using the command calcTPVotes. The option 'minFit' tells the MTEX that the only those triple junctions are considered where the fit to the common parent orientation does not exceed 2.5 degree.

The above command does not only compute the best fitting but also the second best fitting parent orientation. This allows us to ignore ambigues triple points which may vote equally well for different parent orientations. In the above command we did this by the option 'maxFit' which tells MTEX to ignore all triple points where the fit to the second best parent orientation is below 5 degree.

From all remaining triple points the command calcTPVotes compute a list of votes stored in job.votes that contain for each child grain the most likely parent orientation and a corresponding probability job.votes.prob. We may visualize this probability for each grain

We observe that for most of the grains the probability is above 70 percent. We may use this percentage as threshold to decide which child grains we turn into parent grains. This can be done by the command command calcParentFromVote

We observe that after this step more then 66 percent of the grains became parent grains. Lets visualize these reconstructed beta grains

## Grow parent grains at grain boundaries

Next we may grow the reconstructed parent grains into the regions of the remaining child grains. To this end we use the command calcGBVotes with the option 'p2c' to compute votes from parent to child grain boundaries. Next we use the exact same command calcParentFromVote to recover parent orientations from the votes. As threshold for the growing the parent grains into the child grains we use 2.5 degree, 5 degree and 7.5 degree. This can be easily accomblished by the following small loop.

## Merge parent grains

After the previous steps we are left with many very similar parent grains. In order to merge all similarly oriented grains into large parent grains one can use the command mergeSimilar. It takes as an option the threshold below which two parent grains should be considered a a single grain.

## Merge inclusions

We may be still a bit unsatisfied with the result as the large parent grains contain a lot of poorly indexed inclusions where we failed to assign a parent orientation. We use the command mergeInclusions to merge all inclusions that have fever pixels then a certain threshold into the surrounding parent grains.

## Reconstruct beta orientations in EBSD map

Until now we have only recovered the beta orientations as the mean orientations of the beta grains. In this section we want to set up the EBSD variable parentEBSD to contain for each pixel a reconstruction of the parent phase orientation. This is done by the command calcParentEBSD

The recovered EBSD variable parentEBSD contains a measure parentEBSD.fit for the corespondence between the beta orientation reconstructed for a single pixel and the beta orientation of the grain. Lets visualize this

For comparison the map with original alpha phase and on top the recovered beta grain boundaries