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This is Part 2 of the preceding TTL BL page.
TTL BL exposure is influenced by four factors, other than any normal metering of the scene:
In contrast, TTL mode is only affected by #4, i.e., TTL mode does NOT watch the others automatically (and someone has to watch 1-3, but it helps to be there, and see it). The others (1-3) are considered helpful automation for TTL BL mode (point&shoot), but sometimes cause their own problems.
This page looks at #3, D-lens distance. Sometimes D-lens data reports shorter than the actual distance.
The TTL BL D-lens algorithm is that when the metered flash attempts to use more power than Guide Number says is appropriate for the distance (maybe TTL BL metered a distant dark background), TTL BL pulls the flash power back to match the D-lens reported distance (a safety factor preventing overexposure, computed with Guide Number). Problem is, D-lens distance is crude, and some lenses are simply not correct, and none are precise. TTL BL exposure depends on metered value, but if the Reported lens distance is less than actual distance, then flash level will be pulled back (TTL BL direct flash only). If Reported distance is Infinity, or any value greater than actual distance, then the undisturbed metered value is used. I am making this next part up, but FWIW, my notion is thinking there may be a limit to the maximum correction allowed due to D-lens. Some of the results are bad, but not quite as bad as the numbers would suggest.
The SB-400, SB-700, the internal flash, and Commander remote flashes do only TTL BL by system default (when their menu selects the the generic TTL (Through The Lens metering), it is TTL BL. The Exif reports TTL BL (in the Exif Flash Data section, at the end - but Adobe omits that. Check your original file with another Exif viewer.) Spot metering does override any TTL BL to be TTL (but it also does Spot metering too).
Flash GN mode is shown as a comparison, because it is usually about accurate exposure for direct flash, when the accurate actual measured distance is given to GN mode. My notion is that GN mode is what it probably ought to look like. GN mode and TTL mode are not affected by D-lens distance, but the D lens reported value is still shown here, to indicate that sometimes it is variable at each shutter press (focus seeking I think). The camera focuses by rotating the lens for the best appearance in the pixels.
Reports on two lenses are here. Both are prized as great lenses, but the Nikon 16-85mm is no prize regarding D-lens distance. Nor is the Nikon 12-24, but the Nikon 14-24mm is, because it generally just ignores it and reports infinity. One point is to show the obvious difference (below) that it makes to TTL BL direct flash (same camera, same flash, same subject, same situation). It was carefully done, however there are variances, doing any of it twice may see two distance results (focus seeking). Also there are are few unexplained variations, so not every sample fits the plan, but most do.
Situation for all the pictures: Nikon D300 (DX), f/5.6 ISO 200, 1/200 second shutter, matrix metering. SB-800, maximum range is 25 feet at ISO 200 f/5.6. Hot shoe direct flash, focus on white card edge (on the edge, half of the metered area is not white card). 18% gray card also included. The actual distances were carefully measured. The only changes made are as reported, to distance, zoom, flash mode. White Balance is the only correction/compensation done. WCV just means White Card Value from eye dropper.
| GN flash mode | TTL flash mode | TTL BL flash mode |
![]() 16mm zoom at 5 feet (1.5m), reported as 0.8m, WCV 249 |
![]() reported as 1.0m, WCV 246 |
![]() reported as 0.9m, WCV 206 Flash reduced from 1.5m to 0.9m value |
![]() 35mm zoom at 5 feet (1.5m), reported as 1.7m, WCV 242 |
![]() reported as 1.7m, WCV 203 |
![]() reported as 1.7m, WCV 211 Greater than 1.5m, not reduced |
![]() 85mm zoom at 5 feet (1.5m), reported as 1.4m, WCV 238 |
![]() reported as 1.7m, WCV 184 |
![]() reported as 1.7m, WCV 197 |
![]() 16mm zoom at 7.5 feet (2.3m), reported as 1.4m, WCV 252 |
![]() reported as 1.2m, WCV 250 |
![]() reported as 0.9m, WCV 205 |
![]() 35mm zoom at 7.5 feet (2.3m), reported as 2m, WCV 244 |
![]() reported as 2m, WCV 229 |
![]() reported as 2m, WCV 214< |
![]() 85mm zoom at 7.5 feet (2.3m), reported as 1.4m, WCV 246 |
![]() reported as 1.7m, WCV 249 |
![]() reported as 1.7m, WCV 199 |
![]() 16mm zoom at 10 feet (3m), reported as 2m, WCV 255 |
![]() reported as 2.8m, WCV 255 |
![]() reported as 2.8m, WCV 240 |
![]() 35mm zoom at 10 feet (3m), reported as 3.6m, WCV 250 |
![]() reported as 3.6m, WCV 238 |
![]() reported as 3.6m, WCV 223 |
![]() 85mm zoom at 10 feet (3m), reported as 3.6m, WCV 252 |
![]() reported as 3.6m, WCV 205 |
![]() reported as 3.6m, WCV 227 |
![]() 16mm zoom at 12.5 feet (3.8m), reported as 2m, WCV 255 |
![]() reported as 2m, WCV 249 |
![]() reported as 2m, WCV 231 |
![]() 35mm zoom at 12.5 feet (3.8m), reported as 5m, WCV 254 |
![]() reported as 5m, WCV 242 |
![]() reported as 3.6m, WCV 228 |
![]() 85mm zoom at 12.5 feet (3.8m), reported as 3.6m, WCV 253 |
![]() reported as 3.6m, WCV 213 |
![]() reported as 3.6m, WCV 209 |
![]() 16mm zoom at 15 feet (3.8m), reported as 2m, WCV 250 |
![]() reported as 2m, WCV 240 |
![]() reported as 2m, WCV 208 |
![]() 35mm zoom at 15 feet (3.8m), reported as 5m, WCV 244 |
![]() reported as 5m, WCV 235 |
![]() reported as 5m, WCV 213 |
![]() 85mm zoom at 15 feet (3.8m), reported as 5m, WCV 243 |
![]() reported as 5m, WCV 212 |
![]() reported as 5m, WCV 203 |
![]() 16mm zoom at 17.5 feet (5.3m), reported as 2.8m, WCV 246 |
![]() reported as 2m, WCV 220 |
![]() reported as 2m, WCV 176 |
![]() 35mm zoom at 17.5 feet (5.3m), reported as 5m, WCV 242 |
![]() reported as 9.4m, WCV 229 No harm done, it's large, like infinity |
![]() reported as 5m, WCV 202 |
![]() 85mm zoom at 17.5 feet (5.3m), reported as 5m, WCV 242 |
![]() reported as 5m, WCV 218 |
![]() reported as 5m, WCV 194 |
![]() 16mm zoom at 20 feet (5.3m), reported as 3.6m, WCV 244 |
![]() reported as 2.8m, WCV 194 |
![]() reported as 2.8m, WCV 167 |
![]() 35mm zoom at 20 feet (5.3m), reported as 5m, WCV 242 |
![]() reported as 9.4m, WCV 227 |
![]() reported as 5m, WCV 209 |
![]() 85mm zoom at 20 feet (5.3m), reported as 9.4m, WCV 240 |
![]() reported as 5m, WCV 224 |
![]() reported as 5m, WCV 204 |
This lens is the best case I have seen, of non-intrusive D lens info (less harm done to TTL BL direct flash).
| GN flash mode | TTL flash mode | TTL BL flash mode |
![]() 14mm zoom at 5 feet (1.5m), reported as 2m, WCV 249 |
![]() reported as 2m, WCV 246 |
![]() reported as 1.3m, WCV 206 This is limiting |
![]() 18mm zoom at 5 feet (1.5m), reported as 2m, WCV 242 |
![]() reported as 2m, WCV 203 |
![]() reported as infinity, WCV 211 This is not limiting. |
![]() 24mm zoom at 5 feet (1.5m), reported as 2m, WCV 238 |
![]() reported as 2m, WCV 184 |
![]() reported as 2m, WCV 197 |
![]() 14mm zoom at 7.5 feet (2.3m), reported as infinity, WCV 252 |
![]() reported as infinity, WCV 250 |
![]() reported as infinity, WCV 205 |
![]() 18mm zoom at 7.5 feet (2.3m), reported as infinity, WCV 244 |
![]() reported as infinity, WCV 229 |
![]() reported as 2m, WCV 214 |
![]() 24mm zoom at 7.5 feet (2.3m), reported as infinity, WCV 246 |
![]() reported as infinity, WCV 249 |
![]() reported as infinity, WCV 199 |
![]() 14mm zoom at 10 feet (3m), reported as infinity, WCV 255 |
![]() reported as infinity, WCV 255 |
![]() reported as infinity, WCV 240 |
![]() 18mm zoom at 10 feet (3m), reported as infinity, WCV 251 |
![]() reported as infinity, WCV 238 |
![]() reported as infinity, WCV 221 |
![]() 24mm zoom at 10 feet (3m), reported as infinity, WCV 251 |
![]() reported as infinity, WCV 220 |
![]() reported as infinity, WCV 239 |
![]() 14mm zoom at 15 feet (3.8m), reported as infinity, WCV 246 |
![]() reported as infinity, WCV 218 |
![]() reported as infinity, WCV 184 |
![]() 18mm zoom at 15 feet (3.8m), reported as infinity, WCV 244 |
![]() reported as infinity, WCV 235 |
![]() reported as infinity, WCV 213 |
![]() 24mm zoom at 15 feet (3.8m), reported as infinity, WCV 243 |
![]() reported as infinity, WCV 212 |
![]() reported as infinity, WCV 203 |
![]() 14mm zoom at 20 feet (5.3m), reported as infinity, WCV 244 |
![]() reported as infinity, WCV 194 |
![]() reported as infinity, WCV 167 |
![]() 18mm zoom at 20 feet (5.3m), reported as infinity, WCV 242 |
![]() reported as infinity, WCV 227 |
![]() reported as infinity, WCV 209 |
![]() 24mm zoom at 20 feet (5.3m), reported as infinity, WCV 240 |
![]() reported as infinity, WCV 224 |
![]() reported as infinity, WCV 204 |
Clearly better D-lens data (#3 at top of page) gives TTL BL better direct flash results. There is still some built-in bias against TTL BL (#1 & 2 at top of page), but crude D-lens data greatly exaggerates the problems.
Bottom line though, it really doesn't matter much. TTL has other issues too (light reflected from the subject's colors, #4 at top of page), so in all cases, we just watch results and use Flash Compensation as necessary. Just do what you see is necessary. Knowing why helps predict results, but does not change the need.
Then two old non-D lenses. Frankly, my theory was expecting excellent results, and I was greatly surprised to see maybe the worst case yet. These old lenses provide no D-lens data. PhotoME says the 50mm lens "reports" every distance as 0.01 meters, and the 55mm lens reports 0.06 meters (less than 1/4 inch). These are impossible numbers of course, and you'd think this would be known and planned, and expect the system to ignore them, but there is some strong effect. Sorry, no explanation is known, the obvious is unthinkable. Again, same camera, same metering system, same flash, same subject, etc. Only the lens changed.
This lens is from 3 to 5 years before the D-lens era, it does not report it. TTL BL has trouble with this lens.
| GN flash mode | TTL flash mode | TTL BL flash mode |
![]() 5 feet, WCV 221 |
![]() WCV 228 |
![]() WCV 113 |
![]() 10 feet, WCV 245 |
![]() WCV 244 |
![]() WCV 191 |
![]() 15 feet, WCV 242 |
![]() WCV 236 |
![]() WCV 171 |
![]() 20 feet, WCV 239 |
![]() WCV 238 |
![]() WCV 185 |
This manual focus lens is from 25 years before the D-lens era, it does not report it. It is a non-CPU lens, setup in D300 menu. It has been modified to AI mount, to report aperture. TTL BL has trouble with this lens, and TTL is down some too.
| GN flash mode | TTL flash mode | TTL BL flash mode |
![]() 5 feet, WCV 223 |
![]() WCV 197 |
![]() WCV 97 |
![]() 10 feet, WCV 247 |
![]() WCV 202 |
![]() WCV 113 |
![]() 15 feet, WCV 242 |
![]() WCV 202 |
![]() WCV 150 |
![]() 20 feet, WCV 240 |
![]() WCV 219 |
![]() WCV 162 |
My own notion is that we seriously need a menu option to disable effect of D-lens data on TTL BL direct flash.
TTL mode was such an option, but it is disappearing now.
Workarounds:
Sometimes just changing to a lens with more usable D-lens data can make a big difference (see the chart on Previous page, of a few lenses, for example).
Bounce flash is far better lighting anyway (when possible), and bypasses D-lens issues.
If TTL is a choice (SB-600, SB-800, SB-900), it is good stuff. Not always right either of course (because it does meter preflash reflections from the scene), but is consistent, predictable, no unknown programmers messing around mysteriously. Easily predicted and compensated. We do have to know to watch #1-4 at top of this page.
If TTL BL is the only choice, we can compensate results. Or Spot Metering does override TTL BL flash mode to instead be TTL mode, which ignores D-lens distance. However, it is still Spot metering, not simple point&shoot, instead requiring some thought about the spot selected. Spot metering is not general purpose, it does NOT meter the scene, it meters only the spot, and it is an advanced technique requiring more thought.
On cameras with commander, then FV Lock is a feature (for other purposes, to minimize subject blinking for example). But FV Lock can improve the worst TTL BL issues (sometimes giving different and substantially better results), and so also might do a lot to minimize this inaccurate D-lens data problem.
But the bottom line in every case is always Flash Compensation. If you don't like the results, simply fix it. It's pretty easy.
Next is Distant Backgrounds or White Walls are opposite extremes