I absolutely recommend this book. Al Gilbertson spent 30 years researching and interviewing sources. It's eye-opening and really tracks the evolution of the modern round brilliant.Dreamer_D|1392928255|3619494 said:There is also a really cool section in the book American Cut by Al Gilbertson that includes a bunch of examples of diamonds that fell into the Tolk ideal -- the proportions varied a fair bit back then.
http://www.amazon.com/American-Cut-The-First-Years/dp/0873110595
Tolkowsky's book actually put forward six proportion sets.teobdl said:I'm wondering what the exact proportions of the 1919 Tolkowsky Ideal cut diamond were, particularly the LGF's, Star% and Table?
Diamond planning and execution was nowhere as sophisticated or consistent as it is today. A strict lab today would reject many old stones for out-of-round, tilted tables and wide variances in crossworking and brillianteering.teobdl said:More importantly, how would the that ideal look in terms of fire and white light return vs today's AGS 000 MRB?
Depends on how you define light return and which obstruction model you would use but it would be close to the top but there would be many in the same ballpark and maybe a few higher leaving the lgf% and girdle the same.teobdl|1392955851|3619861 said:Important question: using todays technology to ray trace, etc., would the proportions of the Tolk ideal (40.75, 34.5, etc) actually give the best light return (keeping the LGF constant, only changing PA-CA-table). Or is there another set of proportions that actually gives better light return for that LGF length?
John Pollard|1392935744|3619609 said:...His calculated "best" was what we consider traditional Tolkowksy measurements: 53T 34.5CA 40.75PA (43.1%PD) with a knife-edge girdle. No LGFs were specified but they were notably shorter in those days. As the gas lantern gave way to electric lighting table sizes got larger and lower halves got longer. And, of course, girdles now provide durability.
teobdl|1392934071|3619570 said:Thanks Dreamer and Karl!
And theoretically speaking, are these really the proportions that maximize performance for that LGF percentage (and maybe even any LGF percentage)?
The reason I ask is that it strikes me as a little strange that even with the LGF's so short in the Tolk ideal, the other proportions have stayed so constant for the MRB.
I'm also trying to make sense of an AVR, which has even shorter LGF's than the Tolk Ideal. To maximize light return for the short LGF's, Rhina went steeper on the pav and crown.
By comparison If you lengthen the LGF's from a Tolk to MRB, I would think that you would have to change something to keep maximal light performance (by which I mean balanced fire, brilliance, and scintillation).
teobdl|1393104803|3620790 said:Rhino--definitely helps. Thanks you. I'd suspected that the obstruction in the center was the reason you went steeper with shorter LGF's. Fig 42 of this AGS article showed a similar ASET pattern to your AVR, but with blues under the table rather than the red. To brighten it in the center, you went along the anti-cutters line (Fig 27,2.
http://www.agslab.com/spie/spie_lo_res.pdf
Now that I see it again, it seems like the 1919 Tolk would show a similar pattern to Fig 42, and go dark in the center when obstructed in real life. This would be exacerbated by the point light sources of the time, rather than today's abundant and diffuse light sources. Hard to think that, given the shorter LGF's, people would prefer Tolk's proportions over Morse's.
The book is on my to-read list.
That is why I said it depends on which obstruction model you use.teobdl|1393104803|3620790 said:Rhino--definitely helps. Thanks you. I'd suspected that the obstruction in the center was the reason you went steeper with shorter LGF's. Fig 42 of this AGS article showed a similar ASET pattern to your AVR, but with blues under the table rather than the red. To brighten it in the center, you went along the anti-cutters line (Fig 27,2.
http://www.agslab.com/spie/spie_lo_res.pdf
Now that I see it again, it seems like the 1919 Tolk would show a similar pattern to Fig 42, and go dark in the center when obstructed in real life. This would be exacerbated by the point light sources of the time, rather than today's abundant and diffuse light sources. Hard to think that, given the shorter LGF's, people would prefer Tolk's proportions over Morse's.
The book is on my to-read list.
lol.. at least they didn't give the angles away later in the article using one from their charts instead with a larger table.Rhino|1393107513|3620809 said:PS: I see they put an Octavia in that AGS article too! What's funny is they refer to it as a "high performing emerald cut".
Karl_K|1393112494|3620836 said:lol.. at least they didn't give the angles away later in the article using one from their charts instead with a larger table.Rhino|1393107513|3620809 said:PS: I see they put an Octavia in that AGS article too! What's funny is they refer to it as a "high performing emerald cut".
It is also clear the scanner did not get a very good scan of the Octavia.