daan wrote: ↑Wed Apr 26, 2023 7:25 amAngular deformation is independent of nominal scale. Areal inflation and deflation (flation) have to be referred to something. A way to avoid nominal scale as the reference would be to compute the measure against the greatest or least scale factor in the map. However, the least scale in some maps is zero, so that technique fails there, and it’s infinite in many maps, and so fails in those maps as well. Nominal scale ends up being the usual choice.
Or you could use
the second-derivative-ish measure of areal distortion that we ended up discussing a few months later.
justlikeoldtimes wrote: ↑Sat Mar 09, 2024 9:51 pmBut this is what I did a year ago before my mind wandered off. I don't feel the need even label these, considering the crowd here.
Haha, nope!
I'm particularly intrigued by the Collignon one. I wouldn't consider either of them to be good projections, and yet they're apparently bad in about the same ways, since the animation shows remarkably little difference between them. I assume this is to the similarity to the sinusoidal projection (which is a little more curvy, but also has angular poles), which is the one projection that, per definition, would end up with a completely static "animation" in this series.
I'm also interested in the Mollweide/Apian one, which, since Mollweide is a projection that I actually like using, and also common in scientific literature, despite having no read theoretical basis for this (no, Earth
isn't actually a 2:1 ellipse). The relatively significant differences between the two (particularly over Africa) do highlight the limitations of trying to map Earth as an ellipse, despite it feeling intuitively "right". Then again, it still doesn't look as severe as the azimuthal projections.