Hi,

Sorry for such a long message, but I think,
it's really a tough topic, which is so
interlinked that it can't be split into pieces.

Since quite a while I'm trying to get started
with the new modules in darktable 3, but
without success. The promise of gracefully
dealing with high dynamic range scenes, on the
other hand, is really seductive.

I've watched Aurelien Pierre's videos several
times and searched the net for answers, but
only got the impression, that most aren't doing
so much better than myself. Everything seems to
indicate that this can't be learned without a
considerable amount of understanding, while all
these modules are less artistic than technical,
mathematical issues. This, in spite of some
obvious efforts to make it 'easy to use' (which
actually complicates matters, as it makes it
harder to understand the inner workings, or
matching concepts about color science, I've
already learned in a different context).

I think to have understood, that exposure,
filmic and tone equalizer are there to map the
scene's dynamic into a range of intensities
that fits into the dynamic, the internal color
space is able to work with. At the beginning I
though that 'linear RGB' meant some sort of
radiometric proportionality, but reading some
Wikipedia articles about ACES tells me that
this should all be in the photometric domain.
But it is sort of a mixture, at least in my
head, as the exposure module comes very early
in the pixel pipe, is declared to work with
linear RBG but uses EV units, which are a
logarithmic concept. I'm using a self made ICC
camera profile, which I always thought of
dealing with photometric entities. On the other
hand, there are many articles pointing out,
that a 'gamma transform' is an inheritance of
the cathode ray tube monitors, which today
isn't really needed anymore and, if used, will
be undone before lighting up a LED on a modern
monitor. So what is the color space, which the
exposure module is working in, actually linear
to? Filmic's S-shaped curve reminds terribly of
the gamma correction. Aren't photometric
entities already adjusted for the behaviour of
the human eye and brain?

Being a technical/mathematical issue, it must
be possible to state a goal which should be
achieved with each of these three modules.

I believe to have understood, that the black
level correction in exposure must be so low as
to avoid zero or negative RGB values later, in
a more logarithmic domain. So the goal might be
just to accept the setting which can be found
by clicking on the pipette icon near ''clipping
threshold'', no matter how washed out the image
might look.

If that lowest level of intensities is fixed,
any change of exposure in the same module needs
to perform some sort of uniform compression or
dilation. But the drawings in one of Aurelien
Pierre's videos seem to suggest a more linear
shift of the scene's dynamic range with regard
to the dynamic range of the internal working
color space. Where did I miss the turn?

At one point, Mr. Aurelien Pierre states, that
one can either try to fit the highest
intensities into the histogram, or trying to
set the mid tones right, even if this makes the
highest intensities appear overexposed; it
wouldn't matter. At another point he says, that
it's the second option which should be chosen,
which may be in sync with the fact that in the
later versions of filmic:scene, the setting of
the middle grey is already only optional, as
that should have been done before in the
exposure module. For that, I should (mentally)
adjust the exposure module, such that a
rectangle within the image, enclosing an area
which in the scene has about the same
brightness as my grey card, yields something
close 18.42%. If this was right, I wonder, why
the exposure module doesn't have a function
similar to the fulcrum pipette in color
balance. So, what is the goal I have to look
for, such that the following modules allow for
a successful adjustment? If the exposure module
with regard to some unknown rules is rather
off, there is no chance to get the other
modules right. I've found out that much.

I've found even less clues for the final goal
in the filmic rgb module. I think I did
understand, that it is the shape of the
S-curve, which marks the transition of the
linear to a more logarithmic distribution of
the intensities. Beyond that, I'm really lost.
Where should I start? The module opens with the
scene-tab, but the look-tab already has some
settings that directly affect the effect of
the white and black relative exposures. Both
tabs together have 7 parameters. Just trying to
guess a combination of them that 'looks good to
my eye' is really difficult. As a matter of
fact, watching the videos, Aurelien Pierre also
switches back and forth many times, the only
difference beeing, that he does know exactly
what he's doing and being successful, and I
don't. So, where do I start, and what should I
look out for at each point?

Also the tone equalizer seems to be much easier
when Aurelien Pierre is using it. In the live
video, one of the guests mention that 'the mask
interface needs some more love'. I couldn't
agree more! I've tried to do something like in
the video, but there are so many cases where
two areas in the image fall within the same
range of EV but should be adjusted differently.

Excited by the promise, being able to deal with
high dynamic ranges, I shot a bracket of my
living room, having weak but direct sunlight
caught in the curtains at one side, and a
rather dark corridor at the other. A second
image was of a building's front. The sunlight
came almost straight at 90 degrees from a side,
not falling on the building, but there is a mid
sized object in front of the building at an
angle, picking up a rather harsh light.
Nevertheless, besides some tiny spots, the
image isn't overexposed on the sensor (as
indicated by darktable). I wasn't able to
improve any of these to cases. Switching
between the original image, each step in the
history stack seems to make it worse.

I don't want someone fixing these images for
me; these are only for learning. I'm asking for
explanations that will allow me to fix these
and all other images I'm (not yet) planing to
shoot. The main question is: what goal do I
need to achieve at each point?

I'm convinced, that there must be many users of
darktable out there, struggling with these new
issues.
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