Fair enough. I will need to order this lens and test it in my own set up. I will expand the order for additional lenses if it performs as I hope. I will post the specifics of the set up and the beam specs to let others judge for them selves as to whether it might work for them.
At the risk of being critical, I think you might be able to simplify this issue. I believe it is fair and useful to consider the near field to be "within the projector" so 10 to 20 cm might be a reasonable starting point. Because it splits the two distances and is typical of most indoor applications, let me specify the far field at 15M. The telescope would be placed at an arbitrary point prior to a scanner and so somewhat less than 10 to 20 cm. The type of telescope weather prism or cylinder I do not believe is significant, however your choice is fine, theoretically.
I present the comparison in this way in order to bypass the issue of terminology. In my experience EVERY TIME I have manipulated a laser beam in the near field by reducing or enlarging its collimated diameter with refractive optics its far field spot size has enlarged or decreased to an extent that is inversely proportional and linear,
Looking over your plots carefully, I would say the the average power density of the aspheric lens is 3X that of the O-like even ignoring any difference in overall power throughput! The power density at 5M is slightly higher for the aspheric as well. Do you see what I am getting at?
Andy,
We are assuming the lens used does not introduce any aberrations such as when a short FL sphere introduces significant spherical aberration. And that is my question. Do we pursue ever shorter and shorter FL aspheres because they will somehow better correct the asymmetries of these high aspect emitters?