That is exactly the point I was trying to make. You make the reading that you can see. Let's say it happens to be the brightness you would like to see in Zone VI. Do you place it in Zone X on the paper? Not likely. You want some headroom for accents, etc. It doesn't matter if you can see the lower and higher Zones or not, you can still expose that brightness as if it were Zone VI. After all, the other values of SBR may be in areas too small to get a proper reading with the meter at hand. We do such things often. If we spy an area that looks to be the same brightness we're concerned with, we substitute it for the meter reading. Or we read something we judge to be a certain number of Zones higher or lower but is large enough to be measurable. Now why must we change that part of our technique just because the light is too dim to allow exposing the precise area we want to be in a certain Zone? What other mystery does reciprocity hold for us than requiring more exposure time? Is there some different time that must be added to each brightness? If there is, there is no way we can do it. At least not without resorting to the evil of digital computation and a digitally controlled scanning device in place of the shutter. That is why the film speed, CI, Zone or related systams, etc were invented and are used. Now we forget all that because we are worried "What if the characteristic curve changes with long exposure times?" I contend that if you know the Zone you want to use to print whatever part of the scene you can see, you can use the exposure you would normally calculate with your meter for that Zone I and f/stop, and add the correction for reciprocity to that time. If you do learn that for a given film the CI for given development varies with exposure time, you cannot change that by changing exposure time. It can only be changed by development.