The original definition? How about defining that?
1. Three widely spaced wavelengths are brought to the same focus.
2. Two of the wavelengths are corrected for SA and Coma.
3. One of the crossing points for color correction coincides with one of the crossing points for SA and Coma and this crossing point is as close as possible to the Fraunhofer e-line.
FYI, I did the underlining to show that there is wiggle room even in Abbe's original definition. And you see this in practice because for those manufacturers that publish their color crossing data, the wavelengths are always changing 
But as Thomas Back pointed out, what is the purpose of this definition in visual astronomy? Of course it is to achieve a visually CA free image. So that being the case, there are other definitions that meet this outcome for visual observers, such as:
1. Any lens, be it a doublet, triplet, quad, air-spaced or Petzval
2. Has a peak visual null (~5550A - the green-yellow) with a Strehl ratio of .95 or better
3. Coma corrected
4. Diffraction limited from C (red) to F (blue) with 1/4 wave OPD spherical or better
5. Has good control of the violet g wavelength with no more than 1/2 wave OPD P-V spherical and optical spot sizes that concentrate the maximum amount of photons within the diffraction limit
IMO, the use of Apochromat has evolved for astronomy to simply mean color free visually. Whether one likes it or not, that is what the popular usage is evolving into. Language evolves. Would be interesting to see someone place on an objective "Abbe Apochromat". That would certainly convey that it meets the original definition.
Edited by BillP, 18 June 2015 - 04:37 PM.