  To date at least 10 highly flattened planes of dwarf galaxies are claimed to
have been discovered in the Local Universe. The origin of these planes of
galaxies remains unknown. One suggestion is that they are related to the
large-scale structure of the cosmic web. A recent study found that the normal
of a number of these dwarf galaxy planes are very closely aligned with the
eigenvector of the shear tensor corresponding to the direction of greatest
collapse obtained by reconstructing the full velocity field in the linear
regime. Here we extend that work by both considering an additional 5 planes
beyond the 5 examined previously and by examining the alignment with respect to
the quasi-linear field, a more sophisticated reconstruction, which is a better
approximation on smaller (quasi-linear) scales. Our analysis recovers the
previous result while not finding a significantly tight alignment with the
additional 5 planes. However, the additional 5 planes normals also do not
appear to be randomly oriented. We conclude that this could either be due to
the normals of the new planes being poorly defined and described; the
quasi-linear field at those locations being poorly constrained; or different
formation mechanisms for the orientation of planes of dwarf galaxies.
