Good question. That's the effect of spherochromatism (changes in level of spherical aberration which vary with changes in wavelength, i.e., color). It's impossible to produce refractive optics which focus all colors at the same point and which correct for spherical aberration (SA) equally well in all colors. The optical designer will typically strive to figure the lens so that it has best correction in green (or somewhere close to that), as that's where our eyes are most sensitive. Most well-corrected apochromatic scopes that I've seen have very good correction in red as well, and blue tends to fall a little farther off. If the lens designer tried to perfect the correction in the blue wavelengths of light, red and green would likely look much worse, and I suspect that the scope's visual and photographic images would suffer quite a bit as a result.
A very good answer, but I think the designers today lean towards a 620nm figure for faster scopes that are most likely to be used for imaging. This is because many astro-camera sensors are regular sensors that don't have the IR cut filter on the sensor.
For example, here are some Takahshi 106ED scopes.
The first one is tested 532nm and the Strehl is .91. This was probably a bit unfair because while it is what it is in green light, if the system is optimized for 620nm, this test is under-rating the Strehl, though to be fair, this scope isn't the best that Tak has made. You can clearly see that there is some astigmatism and coma. Now the optical quality is still good, but not what one would expect from a brand that is renowned for its quality. I think the major issue though is they tested a scope that was likely optimized for 620nm at 532nm.
http://fidgor.ru/Obs...t/test_241.html
This second one has been tested at 620nm and the scope does much better with a Strehl of .963
http://fidgor.ru/Obs...t/test_186.html
Another one tested at 620nm, and here we have a really excellent instrument, with a Strhel of .971.
This is sadly not a very good Takahashi, but it I am including it here simply because there is still relevant information. The scope was tested at 632nm, but the amount of coma that is present gives the scope a rather low Strehl for such an expensive brand. The top test chart shows the Strehl to be .888 with the coma, but in the second report, the tester has turned off the coma, which is by far and away the most serious error. The important thing though is that this lets the tester see how good the scope would be if the error was removed and as can be seen, if you look at the correction at 632nm with the coma removed, it is now .958, which would make it in the excellent category.
Coma removed, .958 Strehl
http://fidgor.ru/Obs...st/test_93.html
This last test is probably the most important:
Here, we see that the test was run twice. The first test was done at 53nm and the second test was done at 632nm. The first test is made without deductions for things like coma and astigmatism, and the Strehl at 632nm is .963.
The second test is with the coma removed and the Strehl without this error would be .98. The last test show though is the comparison without deductions at 532nm and note that the Strehl is lower than it was at 632nm, coming int a .938.
I would pay attention to the lower order spherical aberration figure, which is .011 at 632nm and .337 at 532nm. It would appear that this scope is indeed optimized for 632, and I do believe that this has become much more common for scopes where the designer thinks the primary use will be for imaging.
http://fidgor.ru/Obs...t/test_186.html
Scopes that are likely more aimed at visual observers, such as the 125EDL or the SkyWatcher 120ED, are probably more optimized for 532nm.
The reason of course is that while our eye cannot see red fringing as easily as blue, the camera with no IR block filter will see the blue and red as equally bright, but the camera will also see 655nm (H-a) very bright as well.